Radio observations of NGC 6388: an upper limit on the mass of its central black hole
Identifieur interne : 000B54 ( Istex/Corpus ); précédent : 000B53; suivant : 000B55Radio observations of NGC 6388: an upper limit on the mass of its central black hole
Auteurs : D. Cseh ; P. Kaaret ; S. Corbel ; E. Körding ; M. Coriat ; A. Tzioumis ; B. LanzoniSource :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2010-08-01.
English descriptors
- KwdEn :
- 2mass source, Accreting, Accretion, Accretion rate, Arcsec, Atca, Atca radio observations, Australia telescope, Binary, Black hole, Black hole mass, Black holes, Bondi hoyle, Centre, Chandra, Chandra aspect uncertainty, Chandra data, Chandra observation, Chandra sources, Cluster centre, Corbel, Data sets, Deep radio observations, Eddington luminosity, Error circle, Falcke, Fundamental plane, Globular, Globular cluster, Globular clusters, Gravity error circle, Interstellar medium, Intrinsic scatter, Journal compilation, Kaaret, Lanzoni, Luminosity, Maccarone, Miller hamilton, Mnras, More detail, Noise level, Nucita, Photon index, Pixel, Pixel randomization, Pooley rappaport, Portegies zwart, Radio detection, Radio luminosity, Radio observations, Radio source, Radio sources, Rding, Subsequent analyses, Surface density, Upper limit.
- Teeft :
- 2mass source, Accreting, Accretion, Accretion rate, Arcsec, Atca, Atca radio observations, Australia telescope, Binary, Black hole, Black hole mass, Black holes, Bondi hoyle, Centre, Chandra, Chandra aspect uncertainty, Chandra data, Chandra observation, Chandra sources, Cluster centre, Corbel, Data sets, Deep radio observations, Eddington luminosity, Error circle, Falcke, Fundamental plane, Globular, Globular cluster, Globular clusters, Gravity error circle, Interstellar medium, Intrinsic scatter, Journal compilation, Kaaret, Lanzoni, Luminosity, Maccarone, Miller hamilton, Mnras, More detail, Noise level, Nucita, Photon index, Pixel, Pixel randomization, Pooley rappaport, Portegies zwart, Radio detection, Radio luminosity, Radio observations, Radio source, Radio sources, Rding, Subsequent analyses, Surface density, Upper limit.
Abstract
We present the results of deep radio observations with the Australia Telescope Compact Array (ATCA) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the Chandra X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. We discuss the uncertainties of this upper limit and the previously suggested black hole mass of based on surface density profile analysis.
Url:
DOI: 10.1111/j.1365-2966.2010.16726.x
Links to Exploration step
ISTEX:3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDELe document en format XML
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Cseh</name><affiliation><mods:affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</mods:affiliation></affiliation><affiliation><mods:affiliation>E-mail: david.cseh@cea.fr</mods:affiliation></affiliation></author><author><name sortKey="Kaaret, P" sort="Kaaret, P" uniqKey="Kaaret P" first="P." last="Kaaret">P. Kaaret</name><affiliation><mods:affiliation>Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA</mods:affiliation></affiliation></author><author><name sortKey="Corbel, S" sort="Corbel, S" uniqKey="Corbel S" first="S." last="Corbel">S. Corbel</name><affiliation><mods:affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</mods:affiliation></affiliation></author><author><name sortKey="Kording, E" sort="Kording, E" uniqKey="Kording E" first="E." last="Körding">E. Körding</name><affiliation><mods:affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</mods:affiliation></affiliation></author><author><name sortKey="Coriat, M" sort="Coriat, M" uniqKey="Coriat M" first="M." last="Coriat">M. Coriat</name><affiliation><mods:affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</mods:affiliation></affiliation></author><author><name sortKey="Tzioumis, A" sort="Tzioumis, A" uniqKey="Tzioumis A" first="A." last="Tzioumis">A. Tzioumis</name><affiliation><mods:affiliation>Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia</mods:affiliation></affiliation></author><author><name sortKey="Lanzoni, B" sort="Lanzoni, B" uniqKey="Lanzoni B" first="B." last="Lanzoni">B. Lanzoni</name><affiliation><mods:affiliation>Dipartimento di Astronomia, Universita‘ degli Studi di Bologna, via Ranzani 1, I‐ 40127 Bologna, Italy</mods:affiliation></affiliation></author></analytic><monogr></monogr><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><biblScope unit="vol">406</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="1049">1049</biblScope><biblScope unit="page" to="1054">1054</biblScope><biblScope unit="page-count">6</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2010-08-01">2010-08-01</date></imprint><idno type="ISSN">0035-8711</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>2mass source</term><term>Accreting</term><term>Accretion</term><term>Accretion rate</term><term>Arcsec</term><term>Atca</term><term>Atca radio observations</term><term>Australia telescope</term><term>Binary</term><term>Black hole</term><term>Black hole mass</term><term>Black holes</term><term>Bondi hoyle</term><term>Centre</term><term>Chandra</term><term>Chandra aspect uncertainty</term><term>Chandra data</term><term>Chandra observation</term><term>Chandra sources</term><term>Cluster centre</term><term>Corbel</term><term>Data sets</term><term>Deep radio observations</term><term>Eddington luminosity</term><term>Error circle</term><term>Falcke</term><term>Fundamental plane</term><term>Globular</term><term>Globular cluster</term><term>Globular clusters</term><term>Gravity error circle</term><term>Interstellar medium</term><term>Intrinsic scatter</term><term>Journal compilation</term><term>Kaaret</term><term>Lanzoni</term><term>Luminosity</term><term>Maccarone</term><term>Miller hamilton</term><term>Mnras</term><term>More detail</term><term>Noise level</term><term>Nucita</term><term>Photon index</term><term>Pixel</term><term>Pixel randomization</term><term>Pooley rappaport</term><term>Portegies zwart</term><term>Radio detection</term><term>Radio luminosity</term><term>Radio observations</term><term>Radio source</term><term>Radio sources</term><term>Rding</term><term>Subsequent analyses</term><term>Surface density</term><term>Upper limit</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>2mass source</term><term>Accreting</term><term>Accretion</term><term>Accretion rate</term><term>Arcsec</term><term>Atca</term><term>Atca radio observations</term><term>Australia telescope</term><term>Binary</term><term>Black hole</term><term>Black hole mass</term><term>Black holes</term><term>Bondi hoyle</term><term>Centre</term><term>Chandra</term><term>Chandra aspect uncertainty</term><term>Chandra data</term><term>Chandra observation</term><term>Chandra sources</term><term>Cluster centre</term><term>Corbel</term><term>Data sets</term><term>Deep radio observations</term><term>Eddington luminosity</term><term>Error circle</term><term>Falcke</term><term>Fundamental plane</term><term>Globular</term><term>Globular cluster</term><term>Globular clusters</term><term>Gravity error circle</term><term>Interstellar medium</term><term>Intrinsic scatter</term><term>Journal compilation</term><term>Kaaret</term><term>Lanzoni</term><term>Luminosity</term><term>Maccarone</term><term>Miller hamilton</term><term>Mnras</term><term>More detail</term><term>Noise level</term><term>Nucita</term><term>Photon index</term><term>Pixel</term><term>Pixel randomization</term><term>Pooley rappaport</term><term>Portegies zwart</term><term>Radio detection</term><term>Radio luminosity</term><term>Radio observations</term><term>Radio source</term><term>Radio sources</term><term>Rding</term><term>Subsequent analyses</term><term>Surface density</term><term>Upper limit</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present the results of deep radio observations with the Australia Telescope Compact Array (ATCA) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the Chandra X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. We discuss the uncertainties of this upper limit and the previously suggested black hole mass of based on surface density profile analysis.</div></front></TEI><istex><corpusName>wiley</corpusName><keywords><teeft><json:string>chandra</json:string><json:string>mnras</json:string><json:string>arcsec</json:string><json:string>black hole</json:string><json:string>upper limit</json:string><json:string>globular</json:string><json:string>luminosity</json:string><json:string>black hole mass</json:string><json:string>cluster centre</json:string><json:string>fundamental plane</json:string><json:string>black holes</json:string><json:string>accreting</json:string><json:string>rding</json:string><json:string>maccarone</json:string><json:string>globular clusters</json:string><json:string>falcke</json:string><json:string>pixel</json:string><json:string>corbel</json:string><json:string>kaaret</json:string><json:string>nucita</json:string><json:string>lanzoni</json:string><json:string>radio luminosity</json:string><json:string>binary</json:string><json:string>atca</json:string><json:string>chandra sources</json:string><json:string>journal compilation</json:string><json:string>centre</json:string><json:string>globular cluster</json:string><json:string>australia telescope</json:string><json:string>radio observations</json:string><json:string>accretion</json:string><json:string>pixel randomization</json:string><json:string>radio sources</json:string><json:string>noise level</json:string><json:string>accretion rate</json:string><json:string>pooley rappaport</json:string><json:string>atca radio observations</json:string><json:string>chandra aspect uncertainty</json:string><json:string>2mass source</json:string><json:string>deep radio observations</json:string><json:string>chandra observation</json:string><json:string>chandra data</json:string><json:string>miller hamilton</json:string><json:string>portegies zwart</json:string><json:string>radio detection</json:string><json:string>error circle</json:string><json:string>gravity error circle</json:string><json:string>photon index</json:string><json:string>eddington luminosity</json:string><json:string>data sets</json:string><json:string>subsequent analyses</json:string><json:string>intrinsic scatter</json:string><json:string>radio source</json:string><json:string>more detail</json:string><json:string>surface density</json:string><json:string>bondi hoyle</json:string><json:string>interstellar medium</json:string></teeft></keywords><author><json:item><name>D. Cseh</name><affiliations><json:string>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</json:string><json:string>E-mail: david.cseh@cea.fr</json:string></affiliations></json:item><json:item><name>P. Kaaret</name><affiliations><json:string>Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA</json:string></affiliations></json:item><json:item><name>S. Corbel</name><affiliations><json:string>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</json:string></affiliations></json:item><json:item><name>E. Körding</name><affiliations><json:string>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</json:string></affiliations></json:item><json:item><name>M. Coriat</name><affiliations><json:string>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</json:string></affiliations></json:item><json:item><name>A. Tzioumis</name><affiliations><json:string>Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia</json:string></affiliations></json:item><json:item><name>B. Lanzoni</name><affiliations><json:string>Dipartimento di Astronomia, Universita‘ degli Studi di Bologna, via Ranzani 1, I‐ 40127 Bologna, Italy</json:string></affiliations></json:item></author><subject><json:item><lang><json:string>eng</json:string></lang><value>accretion, accretion disks</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>black hole physics</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>globular clusters: general</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>globular clusters: individual: NGC 6388</value></json:item><json:item><lang><json:string>eng</json:string></lang><value>radio continuum: general</value></json:item></subject><articleId><json:string>MNR16726</json:string></articleId><arkIstex>ark:/67375/WNG-57BGZLXQ-B</arkIstex><language><json:string>eng</json:string></language><originalGenre><json:string>article</json:string></originalGenre><abstract>We present the results of deep radio observations with the Australia Telescope Compact Array (ATCA) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the Chandra X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. We discuss the uncertainties of this upper limit and the previously suggested black hole mass of based on surface density profile analysis.</abstract><qualityIndicators><refBibsNative>true</refBibsNative><abstractWordCount>124</abstractWordCount><abstractCharCount>732</abstractCharCount><keywordCount>5</keywordCount><score>8.488</score><pdfWordCount>5095</pdfWordCount><pdfCharCount>26296</pdfCharCount><pdfVersion>1.4</pdfVersion><pdfPageCount>6</pdfPageCount><pdfPageSize>595.274 x 782.286 pts</pdfPageSize></qualityIndicators><title>Radio observations of NGC 6388: an upper limit on the mass of its central black hole</title><genre><json:string>article</json:string></genre><host><title>Monthly Notices of the Royal Astronomical Society</title><language><json:string>unknown</json:string></language><doi><json:string>10.1111/(ISSN)1365-2966</json:string></doi><issn><json:string>0035-8711</json:string></issn><eissn><json:string>1365-2966</json:string></eissn><publisherId><json:string>MNR</json:string></publisherId><volume>406</volume><issue>2</issue><pages><first>1049</first><last>1054</last><total>6</total></pages><genre><json:string>journal</json:string></genre></host><namedEntities><unitex><date><json:string>5700</json:string><json:string>2005</json:string><json:string>1970s</json:string><json:string>2003</json:string><json:string>2010</json:string></date><geogName></geogName><orgName><json:string>ATCA</json:string><json:string>Australia Telescope National Facility, CSIRO, PO Box</json:string><json:string>University of Iowa</json:string><json:string>Italy Accepted</json:string><json:string>Australia Telescope Compact Array</json:string></orgName><orgName_funder></orgName_funder><orgName_provider></orgName_provider><persName><json:string>Allen Hall</json:string><json:string>B. 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(2001)</json:string><json:string>Corbel, Tomsick & Kaaret 2006</json:string></ref_bibl><bibl></bibl></unitex></namedEntities><ark><json:string>ark:/67375/WNG-57BGZLXQ-B</json:string></ark><categories><wos><json:string>1 - science</json:string><json:string>2 - astronomy & astrophysics</json:string></wos><scienceMetrix><json:string>1 - natural sciences</json:string><json:string>2 - physics & astronomy</json:string><json:string>3 - astronomy & astrophysics</json:string></scienceMetrix><scopus><json:string>1 - Physical Sciences</json:string><json:string>2 - Earth and Planetary Sciences</json:string><json:string>3 - Space and Planetary Science</json:string><json:string>1 - Physical Sciences</json:string><json:string>2 - Physics and Astronomy</json:string><json:string>3 - Astronomy and Astrophysics</json:string></scopus><inist><json:string>1 - sciences appliquees, technologies et medecines</json:string><json:string>2 - sciences exactes et technologie</json:string><json:string>3 - terre, ocean, espace</json:string><json:string>4 - astronomie</json:string></inist></categories><publicationDate>2010</publicationDate><copyrightDate>2010</copyrightDate><doi><json:string>10.1111/j.1365-2966.2010.16726.x</json:string></doi><id>3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDE</id><score>1</score><fulltext><json:item><extension>pdf</extension><original>true</original><mimetype>application/pdf</mimetype><uri>https://api.istex.fr/document/3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDE/fulltext/pdf</uri></json:item><json:item><extension>zip</extension><original>false</original><mimetype>application/zip</mimetype><uri>https://api.istex.fr/document/3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDE/fulltext/zip</uri></json:item><istex:fulltextTEI uri="https://api.istex.fr/document/3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDE/fulltext/tei"><teiHeader><fileDesc><titleStmt><title level="a" type="main">Radio observations of NGC 6388: an upper limit on the mass of its central black hole</title></titleStmt><publicationStmt><authority>ISTEX</authority><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><availability><licence>© 2010 The Authors. Journal compilation © 2010 RAS</licence></availability><date type="published" when="2010-08-01"></date></publicationStmt><notesStmt><note type="content-type" subtype="article" source="article" scheme="https://content-type.data.istex.fr/ark:/67375/XTP-6N5SZHKN-D">article</note><note type="publication-type" subtype="journal" scheme="https://publication-type.data.istex.fr/ark:/67375/JMC-0GLKJH51-B">journal</note></notesStmt><sourceDesc><biblStruct type="article"><analytic><title level="a" type="main">Radio observations of NGC 6388: an upper limit on the mass of its central black hole</title><title level="a" type="short">The mass of the black hole in NGC 6388</title><author xml:id="author-0000" role="corresp"><persName><forename type="first">D.</forename><surname>Cseh</surname></persName><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France<address><country key="FR"></country></address></affiliation><affiliation>E‐mail: david.cseh@cea.fr</affiliation></author><author xml:id="author-0001"><persName><forename type="first">P.</forename><surname>Kaaret</surname></persName><affiliation>Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA<address><country key="US"></country></address></affiliation></author><author xml:id="author-0002"><persName><forename type="first">S.</forename><surname>Corbel</surname></persName><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0003"><persName><forename type="first">E.</forename><surname>Körding</surname></persName><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0004"><persName><forename type="first">M.</forename><surname>Coriat</surname></persName><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France<address><country key="FR"></country></address></affiliation></author><author xml:id="author-0005"><persName><forename type="first">A.</forename><surname>Tzioumis</surname></persName><affiliation>Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia<address><country key="AU"></country></address></affiliation></author><author xml:id="author-0006"><persName><forename type="first">B.</forename><surname>Lanzoni</surname></persName><affiliation>Dipartimento di Astronomia, Universita‘ degli Studi di Bologna, via Ranzani 1, I‐ 40127 Bologna, Italy<address><country key="IT"></country></address></affiliation></author><idno type="istex">3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDE</idno><idno type="ark">ark:/67375/WNG-57BGZLXQ-B</idno><idno type="DOI">10.1111/j.1365-2966.2010.16726.x</idno><idno type="unit">MNR16726</idno><idno type="toTypesetVersion">file:MNR.MNR16726.pdf</idno></analytic><monogr><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="pISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><idno type="book-DOI">10.1111/(ISSN)1365-2966</idno><idno type="book-part-DOI">10.1111/mnr.2010.406.issue-2</idno><idno type="product">MNR</idno><idno type="publisherDivision">ST</idno><imprint><biblScope unit="vol">406</biblScope><biblScope unit="issue">2</biblScope><biblScope unit="page" from="1049">1049</biblScope><biblScope unit="page" to="1054">1054</biblScope><biblScope unit="page-count">6</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2010-08-01"></date></imprint></monogr></biblStruct></sourceDesc></fileDesc><profileDesc><abstract xml:lang="en" style="main"><head>ABSTRACT</head><p>We present the results of deep radio observations with the Australia Telescope Compact Array (<hi rend="italic">ATCA</hi>) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the <hi rend="italic">Chandra</hi> X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M<graphic url="equation/MNR_16726_mu1.gif" rend="inline image"></graphic> on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. 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E‐mail: <email>david.cseh@cea.fr</email></correspondenceTo><linkGroup><link type="toTypesetVersion" href="file:MNR.MNR16726.pdf"></link></linkGroup></publicationMeta><contentMeta><unparsedEditorialHistory>Accepted 2010 March 22. Received 2010 March 22; in original form 2010 February 16</unparsedEditorialHistory><countGroup><count type="figureTotal" number="2"></count><count type="tableTotal" number="1"></count><count type="formulaTotal" number="95"></count><count type="referenceTotal" number="54"></count><count type="linksCrossRef" number="108"></count></countGroup><titleGroup><title type="main">Radio observations of NGC 6388: an upper limit on the mass of its central black hole</title><title type="shortAuthors"><i>D. Cseh et al.</i></title><title type="short"><i>The mass of the black hole in NGC 6388</i></title></titleGroup><creators><creator creatorRole="author" xml:id="cr1" affiliationRef="#a1" corresponding="yes"><personName><givenNames>D.</givenNames><familyName>Cseh</familyName></personName></creator><creator creatorRole="author" xml:id="cr2" affiliationRef="#a2"><personName><givenNames>P.</givenNames><familyName>Kaaret</familyName></personName></creator><creator creatorRole="author" xml:id="cr3" affiliationRef="#a1"><personName><givenNames>S.</givenNames><familyName>Corbel</familyName></personName></creator><creator creatorRole="author" xml:id="cr4" affiliationRef="#a1"><personName><givenNames>E.</givenNames><familyName>Körding</familyName></personName></creator><creator creatorRole="author" xml:id="cr5" affiliationRef="#a1"><personName><givenNames>M.</givenNames><familyName>Coriat</familyName></personName></creator><creator creatorRole="author" xml:id="cr6" affiliationRef="#a3"><personName><givenNames>A.</givenNames><familyName>Tzioumis</familyName></personName></creator><creator creatorRole="author" xml:id="cr7" affiliationRef="#a4"><personName><givenNames>B.</givenNames><familyName>Lanzoni</familyName></personName></creator></creators><affiliationGroup><affiliation xml:id="a1" countryCode="FR"><unparsedAffiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</unparsedAffiliation></affiliation><affiliation xml:id="a2" countryCode="US"><unparsedAffiliation>Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA</unparsedAffiliation></affiliation><affiliation xml:id="a3" countryCode="AU"><unparsedAffiliation>Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia</unparsedAffiliation></affiliation><affiliation xml:id="a4" countryCode="IT"><unparsedAffiliation>Dipartimento di Astronomia, Universita‘ degli Studi di Bologna, via Ranzani 1, I‐ 40127 Bologna, Italy</unparsedAffiliation></affiliation></affiliationGroup><keywordGroup xml:lang="en"><keyword xml:id="k1">accretion, accretion disks</keyword><keyword xml:id="k2">black hole physics</keyword><keyword xml:id="k3">globular clusters: general</keyword><keyword xml:id="k4">globular clusters: individual: NGC 6388</keyword><keyword xml:id="k5">radio continuum: general</keyword></keywordGroup><abstractGroup><abstract type="main" xml:lang="en"><title type="main">ABSTRACT</title><p>We present the results of deep radio observations with the Australia Telescope Compact Array (<i>ATCA</i>) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the <i>Chandra</i> X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M<inlineGraphic alt="inline image" location="equation/MNR_16726_mu1.gif" href=""></inlineGraphic> on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. We discuss the uncertainties of this upper limit and the previously suggested black hole mass of <inlineGraphic alt="inline image" location="equation/MNR_16726_mu2.gif" href=""></inlineGraphic> based on surface density profile analysis.</p></abstract></abstractGroup></contentMeta></header></component></istex:document></istex:metadataXml><mods version="3.6"><titleInfo lang="en"><title>Radio observations of NGC 6388: an upper limit on the mass of its central black hole</title></titleInfo><titleInfo type="abbreviated" lang="en"><title>The mass of the black hole in NGC 6388</title></titleInfo><titleInfo type="alternative" contentType="CDATA" lang="en"><title>Radio observations of NGC 6388: an upper limit on the mass of its central black hole</title></titleInfo><name type="personal"><namePart type="given">D.</namePart><namePart type="family">Cseh</namePart><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</affiliation><affiliation>E-mail: david.cseh@cea.fr</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">P.</namePart><namePart type="family">Kaaret</namePart><affiliation>Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">S.</namePart><namePart type="family">Corbel</namePart><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">E.</namePart><namePart type="family">Körding</namePart><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">M.</namePart><namePart type="family">Coriat</namePart><affiliation>Laboratoire Astrophysique des Interactions Multi‐echelles (UMR 7158), CEA/DSM‐CNRS‐Universite Paris Diderot, CEA Saclay, F‐91191 Gif sur Yvette, France</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">A.</namePart><namePart type="family">Tzioumis</namePart><affiliation>Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 1710, Australia</affiliation><role><roleTerm type="text">author</roleTerm></role></name><name type="personal"><namePart type="given">B.</namePart><namePart type="family">Lanzoni</namePart><affiliation>Dipartimento di Astronomia, Universita‘ degli Studi di Bologna, via Ranzani 1, I‐ 40127 Bologna, Italy</affiliation><role><roleTerm type="text">author</roleTerm></role></name><typeOfResource>text</typeOfResource><genre type="article" displayLabel="article" authority="ISTEX" authorityURI="https://content-type.data.istex.fr" valueURI="https://content-type.data.istex.fr/ark:/67375/XTP-6N5SZHKN-D">article</genre><originInfo><publisher>Blackwell Publishing Ltd</publisher><place><placeTerm type="text">Oxford, UK</placeTerm></place><dateIssued encoding="w3cdtf">2010-08-01</dateIssued><edition>Accepted 2010 March 22. Received 2010 March 22; in original form 2010 February 16</edition><copyrightDate encoding="w3cdtf">2010</copyrightDate></originInfo><language><languageTerm type="code" authority="rfc3066">en</languageTerm><languageTerm type="code" authority="iso639-2b">eng</languageTerm></language><physicalDescription><extent unit="figures">2</extent><extent unit="tables">1</extent><extent unit="formulas">95</extent><extent unit="references">54</extent><extent unit="linksCrossRef">108</extent></physicalDescription><abstract lang="en">We present the results of deep radio observations with the Australia Telescope Compact Array (ATCA) of the globular cluster NGC 6388. We show that there is no radio source detected (with an rms noise level of 27 μJy) at the cluster centre of gravity or at the locations of any of the Chandra X‐ray sources in the cluster. Based on the fundamental plane of accreting black holes which is a relationship between X‐ray luminosity, radio luminosity and black hole mass, we place an upper limit of ∼1500 M on the mass of the putative intermediate‐mass black hole located at the centre of NGC 6388. We discuss the uncertainties of this upper limit and the previously suggested black hole mass of based on surface density profile analysis.</abstract><subject lang="en"><genre>keywords</genre><topic>accretion, accretion disks</topic><topic>black hole physics</topic><topic>globular clusters: general</topic><topic>globular clusters: individual: NGC 6388</topic><topic>radio continuum: general</topic></subject><relatedItem type="host"><titleInfo><title>Monthly Notices of the Royal Astronomical Society</title></titleInfo><genre type="journal" authority="ISTEX" authorityURI="https://publication-type.data.istex.fr" valueURI="https://publication-type.data.istex.fr/ark:/67375/JMC-0GLKJH51-B">journal</genre><identifier type="ISSN">0035-8711</identifier><identifier type="eISSN">1365-2966</identifier><identifier type="DOI">10.1111/(ISSN)1365-2966</identifier><identifier type="PublisherID">MNR</identifier><part><date>2010</date><detail type="volume"><caption>vol.</caption><number>406</number></detail><detail type="issue"><caption>no.</caption><number>2</number></detail><extent unit="pages"><start>1049</start><end>1054</end><total>6</total></extent></part></relatedItem><identifier type="istex">3D9B41FBFDF251514AA0CFB33DF60EBB21CD1DDE</identifier><identifier type="ark">ark:/67375/WNG-57BGZLXQ-B</identifier><identifier type="DOI">10.1111/j.1365-2966.2010.16726.x</identifier><identifier type="ArticleID">MNR16726</identifier><accessCondition type="use and reproduction" contentType="copyright">© 2010 The Authors. 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