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A CH3CN and HCO+ survey towards southern methanol masers associated with star formation

Identifieur interne : 00A132 ( Main/Exploration ); précédent : 00A131; suivant : 00A133

A CH3CN and HCO+ survey towards southern methanol masers associated with star formation

Auteurs : C. R. Purcell [Australie] ; R. Balasubramanyam [Australie, Inde] ; M. G. Burton [Australie] ; A. J. Walsh [Australie] ; V. Minier [Australie, France] ; M. R. Hunt-Cunningham [Australie] ; L. L. Kedziora-Chudczer [Australie] ; S. N. Longmore [Australie] ; T. Hill [Australie] ; I. Bains [Australie] ; P. J. Barnes [Australie] ; A. L. Busfield [Royaume-Uni] ; P. Calisse [Australie, Royaume-Uni] ; N. H. M. Crighton [Australie] ; S. J. Curran [Australie] ; T. M. Davis [Australie] ; J. T. Dempsey [Australie] ; G. Derragopian [Australie] ; B. Fulton [Australie] ; M. G. Hidas [Australie] ; M. G. Hoare [Royaume-Uni] ; J.-K. Lee [Australie, Royaume-Uni] ; E. F. Ladd [Australie, États-Unis] ; S. L. Lumsden [Royaume-Uni] ; T. J. T. Moore [Royaume-Uni] ; M. T. Murphy [Australie, Royaume-Uni] ; R. D. Oudmaijer [Australie] ; M. B. Pracy [Australie] ; J. Rathborne [Australie, États-Unis] ; S. Robertson [Australie] ; A. S. B. Schultz [Australie] ; J. Shobbrook [Australie] ; P. A. Sparks [Australie] ; J. Storey [Australie] ; T. Travouillion [Australie, États-Unis]

Source :

RBID : Pascal:06-0182663

Descripteurs français

English descriptors

Abstract

ABSIRACT We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected massive star-forming regions. Here, we report observations of the J = 5-4 and 6-5 rotational transitions of methyl cyanide (CH3CN) and the J = 1-0 transition of HCO+ and H13CO+. CH3CN emission is detected in 58 sources (70 per cent of our sample). We estimate the temperature and column density for 37 of these using the rotational diagram (RD) method. The temperatures we derive range from 28-166 K, and are lower than previously reported temperatures, derived from higher J transitions. We find that CH3CN is brighter and more commonly detected towards ultracompact H II (UCH II) regions than towards isolated maser sources. Detection of CH3CN towards isolated maser sources strongly suggests that these objects are internally heated and that CH3CN is excited prior to the UCH II phase of massive star formation. HCO+ is detected towards 82 sources (99 per cent of our sample), many of which exhibit asymmetric line profiles compared to H13CO+. Skewed profiles are indicative of inward or outward motions, however, we find approximately equal numbers of red- and blue-skewed profiles among all classes. Column densities are derived from an analysis of the HCO+ and H13CO+ line profiles. 80 sources have mid-infrared (mid-IR) counterparts: 68 seen in emission and 12 seen in absorption as 'dark clouds'. Seven of the 12 dark clouds exhibit asymmetric HCO+ profiles, six of which are skewed to the blue, indicating infalling motions. CH3CN is also common in dark clouds, where it has a 90 per cent detection rate.


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Le document en format XML

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<s1>Research School of Astronomy and Astrophysics, The Australian National University, Mount Stromlo Observatory, Cotter Road</s1>
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<s1>Centre for Astronomy, James Cook University</s1>
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<s1>Department of Pure and Applied Physics, Queen's University</s1>
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<s1>CSIRO Australia Telescope National Facility, PO Box 76</s1>
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<s1>School of Physics, University of New South Wales</s1>
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<s1>Department of Physics, Bucknell University</s1>
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<name sortKey="Lumsden, S L" sort="Lumsden, S L" uniqKey="Lumsden S" first="S. L." last="Lumsden">S. L. Lumsden</name>
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<s1>School of Physics and Astronomy, University of Leeds</s1>
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<s1>Astrophysics Research Institute, Liverpool John Moores University, 12 Quays House, Egerton Wharf</s1>
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<s1>Institute of Astronomy, University of Cambridge, Madingley Road</s1>
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<s1>Institute for Astrophysical Research, Boston University</s1>
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<name sortKey="Robertson, S" sort="Robertson, S" uniqKey="Robertson S" first="S." last="Robertson">S. Robertson</name>
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<name sortKey="Shobbrook, J" sort="Shobbrook, J" uniqKey="Shobbrook J" first="J." last="Shobbrook">J. Shobbrook</name>
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<name sortKey="Sparks, P A" sort="Sparks, P A" uniqKey="Sparks P" first="P. A." last="Sparks">P. A. Sparks</name>
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<name sortKey="Storey, J" sort="Storey, J" uniqKey="Storey J" first="J." last="Storey">J. Storey</name>
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<name sortKey="Travouillion, T" sort="Travouillion, T" uniqKey="Travouillion T" first="T." last="Travouillion">T. Travouillion</name>
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<s1>School of Physics, University of New South Wales</s1>
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<country>Australie</country>
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<s1>California Institute of Technology, 1200 E. California Blvd</s1>
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<title xml:lang="en" level="a">A CH
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CN and HCO
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survey towards southern methanol masers associated with star formation</title>
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<author>
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<s1>California Institute of Technology, 1200 E. California Blvd</s1>
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<series>
<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
<title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title>
<idno type="ISSN">0035-8711</idno>
<imprint>
<date when="2006">2006</date>
</imprint>
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<title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title>
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</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Abundance</term>
<term>Column density</term>
<term>Dark clouds</term>
<term>HII regions</term>
<term>Line shape</term>
<term>Masers</term>
<term>Massive stars</term>
<term>Methanol</term>
<term>Pre-main-sequence stars</term>
<term>Rotational transition</term>
<term>Star formation</term>
<term>Stellar formation region</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Méthanol</term>
<term>Maser</term>
<term>Formation stellaire</term>
<term>Etoile massive</term>
<term>Région formation stellaire</term>
<term>Transition rotationnelle</term>
<term>Densité colonne</term>
<term>Profil raie</term>
<term>Nuage sombre</term>
<term>Etoile pré séquence principale</term>
<term>Abondance</term>
<term>Région HII</term>
</keywords>
<keywords scheme="Wicri" type="topic" xml:lang="fr">
<term>Méthanol</term>
</keywords>
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<front>
<div type="abstract" xml:lang="en">ABSIRACT We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected massive star-forming regions. Here, we report observations of the J = 5-4 and 6-5 rotational transitions of methyl cyanide (CH
<sub>3</sub>
CN) and the J = 1-0 transition of HCO
<sup>+</sup>
and H
<sup>13</sup>
CO
<sup>+</sup>
. CH
<sub>3</sub>
CN emission is detected in 58 sources (70 per cent of our sample). We estimate the temperature and column density for 37 of these using the rotational diagram (RD) method. The temperatures we derive range from 28-166 K, and are lower than previously reported temperatures, derived from higher J transitions. We find that CH
<sub>3</sub>
CN is brighter and more commonly detected towards ultracompact H II (UCH II) regions than towards isolated maser sources. Detection of CH
<sub>3</sub>
CN towards isolated maser sources strongly suggests that these objects are internally heated and that CH
<sub>3</sub>
CN is excited prior to the UCH II phase of massive star formation. HCO
<sup>+</sup>
is detected towards 82 sources (99 per cent of our sample), many of which exhibit asymmetric line profiles compared to H
<sup>13</sup>
CO
<sup>+</sup>
. Skewed profiles are indicative of inward or outward motions, however, we find approximately equal numbers of red- and blue-skewed profiles among all classes. Column densities are derived from an analysis of the HCO
<sup>+</sup>
and H
<sup>13</sup>
CO
<sup>+</sup>
line profiles. 80 sources have mid-infrared (mid-IR) counterparts: 68 seen in emission and 12 seen in absorption as 'dark clouds'. Seven of the 12 dark clouds exhibit asymmetric HCO
<sup>+</sup>
profiles, six of which are skewed to the blue, indicating infalling motions. CH
<sub>3</sub>
CN is also common in dark clouds, where it has a 90 per cent detection rate.</div>
</front>
</TEI>
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<list>
<country>
<li>Australie</li>
<li>France</li>
<li>Inde</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
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<li>Angleterre</li>
<li>Angleterre de l'Est</li>
<li>Nouvelle-Galles du Sud</li>
<li>Yorkshire-et-Humber</li>
</region>
<settlement>
<li>Cambridge</li>
<li>Leeds</li>
<li>Sydney</li>
</settlement>
<orgName>
<li>Université de Cambridge</li>
<li>Université de Leeds</li>
<li>Université de Sydney</li>
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<name sortKey="Davis, T M" sort="Davis, T M" uniqKey="Davis T" first="T. M." last="Davis">T. M. Davis</name>
<name sortKey="Davis, T M" sort="Davis, T M" uniqKey="Davis T" first="T. M." last="Davis">T. M. Davis</name>
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<name sortKey="Hidas, M G" sort="Hidas, M G" uniqKey="Hidas M" first="M. G." last="Hidas">M. G. Hidas</name>
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<name sortKey="Kedziora Chudczer, L L" sort="Kedziora Chudczer, L L" uniqKey="Kedziora Chudczer L" first="L. L." last="Kedziora-Chudczer">L. L. Kedziora-Chudczer</name>
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<name sortKey="Lee, J K" sort="Lee, J K" uniqKey="Lee J" first="J.-K." last="Lee">J.-K. Lee</name>
<name sortKey="Longmore, S N" sort="Longmore, S N" uniqKey="Longmore S" first="S. N." last="Longmore">S. N. Longmore</name>
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<name sortKey="Robertson, S" sort="Robertson, S" uniqKey="Robertson S" first="S." last="Robertson">S. Robertson</name>
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<name sortKey="Travouillion, T" sort="Travouillion, T" uniqKey="Travouillion T" first="T." last="Travouillion">T. Travouillion</name>
<name sortKey="Walsh, A J" sort="Walsh, A J" uniqKey="Walsh A" first="A. J." last="Walsh">A. J. Walsh</name>
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</affiliations>
</record>

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