Gamma‐ray bursts in normal and extreme star‐forming galaxies
Identifieur interne : 000422 ( Main/Exploration ); précédent : 000421; suivant : 000423Gamma‐ray bursts in normal and extreme star‐forming galaxies
Auteurs : Neil Trentham ; Enrico Ramirez-Ruiz ; A. W. Blain [États-Unis]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2002-08.
English descriptors
Abstract
We discuss how gamma‐ray burst (GRB) optical afterglows and multiwavelength observations of their host galaxies can be used to obtain information about the relative amounts of star formation happening in optical and submillimetre galaxies. That such an analysis will be possible follows from the currently favoured idea that GRBs are closely linked with high‐mass star formation. Studying GRB host galaxies offers a method of finding low‐luminosity submillimetre galaxies, which cannot be identified either in optical Lyman break surveys, because so much of their star formation is hidden by dust, or in submillimetre surveys, because their submillimetre fluxes are close to or below the confusion limit. Much of the star formation in the Universe could have occurred in such objects, so searching for them is an important exercise. From current observations, GRB host galaxies appear to be neither optically luminous Class‐2 SCUBA galaxies like SMM J02399 − 0136 or SMM J14011 + 0252, nor galaxies containing dense molecular cores like local ultraluminous infrared galaxies (ULIGs), but rather some intermediate kind of galaxy. The host galaxy of GRB 980703 is a prototype of this kind of galaxy.
Url:
DOI: 10.1046/j.1365-8711.2002.05586.x
Affiliations:
Links toward previous steps (curation, corpus...)
Le document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Gamma‐ray bursts in normal and extreme star‐forming galaxies</title><author><name sortKey="Trentham, Neil" sort="Trentham, Neil" uniqKey="Trentham N" first="Neil" last="Trentham">Neil Trentham</name></author><author><name sortKey="Ramirez Uiz, Enrico" sort="Ramirez Uiz, Enrico" uniqKey="Ramirez Uiz E" first="Enrico" last="Ramirez-Ruiz">Enrico Ramirez-Ruiz</name></author><author><name sortKey="Blain, A W" sort="Blain, A W" uniqKey="Blain A" first="A. W." last="Blain">A. W. Blain</name></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:3423CD0F99FDE37B10197AE8BBFECF98FD841851</idno><date when="2002" year="2002">2002</date><idno type="doi">10.1046/j.1365-8711.2002.05586.x</idno><idno type="url">https://api.istex.fr/document/3423CD0F99FDE37B10197AE8BBFECF98FD841851/fulltext/pdf</idno><idno type="wicri:Area/Main/Corpus">000688</idno><idno type="wicri:Area/Main/Curation">000688</idno><idno type="wicri:Area/Main/Exploration">000422</idno><idno type="wicri:explorRef" wicri:stream="Main" wicri:step="Exploration">000422</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">Gamma‐ray bursts in normal and extreme star‐forming galaxies</title><author><name sortKey="Trentham, Neil" sort="Trentham, Neil" uniqKey="Trentham N" first="Neil" last="Trentham">Neil Trentham</name><affiliation><wicri:noCountry code="subField">0HA</wicri:noCountry></affiliation></author><author><name sortKey="Ramirez Uiz, Enrico" sort="Ramirez Uiz, Enrico" uniqKey="Ramirez Uiz E" first="Enrico" last="Ramirez-Ruiz">Enrico Ramirez-Ruiz</name><affiliation><wicri:noCountry code="subField">0HA</wicri:noCountry></affiliation></author><author><name sortKey="Blain, A W" sort="Blain, A W" uniqKey="Blain A" first="A. W." last="Blain">A. W. Blain</name><affiliation></affiliation><affiliation wicri:level="1"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Astronomy Department, Caltech 105‐24, Pasadena, CA 91125</wicri:regionArea><wicri:noRegion>CA 91125</wicri:noRegion></affiliation></author></analytic><monogr></monogr><series><title level="j">Monthly Notices of the Royal Astronomical Society</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><publisher>Blackwell Science Ltd</publisher><pubPlace>23 Ainslie Place , Edinburgh EH3 6AJ , UK . Telephone (0131) 226 7232 Fax (0131) 226 3803</pubPlace><date type="published" when="2002-08">2002-08</date><biblScope unit="volume">334</biblScope><biblScope unit="issue">4</biblScope><biblScope unit="page" from="983">983</biblScope><biblScope unit="page" to="989">989</biblScope></imprint><idno type="ISSN">0035-8711</idno></series><idno type="istex">3423CD0F99FDE37B10197AE8BBFECF98FD841851</idno><idno type="DOI">10.1046/j.1365-8711.2002.05586.x</idno><idno type="ArticleID">MNR5586</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>cosmology: observations</term><term>gamma‐rays: bursts</term><term>infrared: galaxies</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We discuss how gamma‐ray burst (GRB) optical afterglows and multiwavelength observations of their host galaxies can be used to obtain information about the relative amounts of star formation happening in optical and submillimetre galaxies. That such an analysis will be possible follows from the currently favoured idea that GRBs are closely linked with high‐mass star formation. Studying GRB host galaxies offers a method of finding low‐luminosity submillimetre galaxies, which cannot be identified either in optical Lyman break surveys, because so much of their star formation is hidden by dust, or in submillimetre surveys, because their submillimetre fluxes are close to or below the confusion limit. Much of the star formation in the Universe could have occurred in such objects, so searching for them is an important exercise. From current observations, GRB host galaxies appear to be neither optically luminous Class‐2 SCUBA galaxies like SMM J02399 − 0136 or SMM J14011 + 0252, nor galaxies containing dense molecular cores like local ultraluminous infrared galaxies (ULIGs), but rather some intermediate kind of galaxy. The host galaxy of GRB 980703 is a prototype of this kind of galaxy.</div></front></TEI><affiliations><list><country><li>États-Unis</li></country></list><tree><noCountry><name sortKey="Ramirez Uiz, Enrico" sort="Ramirez Uiz, Enrico" uniqKey="Ramirez Uiz E" first="Enrico" last="Ramirez-Ruiz">Enrico Ramirez-Ruiz</name><name sortKey="Trentham, Neil" sort="Trentham, Neil" uniqKey="Trentham N" first="Neil" last="Trentham">Neil Trentham</name></noCountry><country name="États-Unis"><noRegion><name sortKey="Blain, A W" sort="Blain, A W" uniqKey="Blain A" first="A. W." last="Blain">A. W. Blain</name></noRegion></country></tree></affiliations></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Amerique/explor/CaltechV1/Data/Main/Exploration
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 000422 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 000422 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/Amerique
|area= CaltechV1
|flux= Main
|étape= Exploration
|type= RBID
|clé= ISTEX:3423CD0F99FDE37B10197AE8BBFECF98FD841851
|texte= Gamma‐ray bursts in normal and extreme star‐forming galaxies
}}
| This area was generated with Dilib version V0.6.32. |  |