Serveur d'exploration sur Caltech

Attention, ce site est en cours de développement !
Attention, site généré par des moyens informatiques à partir de corpus bruts.
Les informations ne sont donc pas validées.

Modelling galaxy clustering: is new physics needed in galaxy formation models?

Identifieur interne : 000128 ( Main/Exploration ); précédent : 000127; suivant : 000129

Modelling galaxy clustering: is new physics needed in galaxy formation models?

Auteurs : Han-Seek Kim ; C. M. Baugh ; S. Cole ; C. S. Frenk ; A. J. Benson [États-Unis]

Source :

RBID : ISTEX:719EBEC207775099DCD192D8FF5FDF90F8CCE622

English descriptors

Abstract

The clustering amplitude of galaxies depends on their intrinsic luminosity. We compare the properties of publicly available galaxy formation models with clustering measurements from the Two‐degree Field Galaxy Redshift Survey. The model predictions show the same qualitative behaviour as the data but fail to match the observations at the level of accuracy at which current measurements can be made. We demonstrate that this is due to the model producing too many satellite galaxies in massive haloes. We implement simple models to describe two new processes: satellite–satellite mergers and the tidal dissolution of satellites to investigate their impact on the predicted clustering. We find that both processes need to be included in order to produce a model which matches the observations.

Url:
DOI: 10.1111/j.1365-2966.2009.15560.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">Modelling galaxy clustering: is new physics needed in galaxy formation models?</title>
<author>
<name sortKey="Kim, Han Eek" sort="Kim, Han Eek" uniqKey="Kim H" first="Han-Seek" last="Kim">Han-Seek Kim</name>
</author>
<author>
<name sortKey="Baugh, C M" sort="Baugh, C M" uniqKey="Baugh C" first="C. M." last="Baugh">C. M. Baugh</name>
</author>
<author>
<name sortKey="Cole, S" sort="Cole, S" uniqKey="Cole S" first="S." last="Cole">S. Cole</name>
</author>
<author>
<name sortKey="Frenk, C S" sort="Frenk, C S" uniqKey="Frenk C" first="C. S." last="Frenk">C. S. Frenk</name>
</author>
<author>
<name sortKey="Benson, A J" sort="Benson, A J" uniqKey="Benson A" first="A. J." last="Benson">A. J. Benson</name>
</author>
</titleStmt>
<publicationStmt>
<idno type="wicri:source">ISTEX</idno>
<idno type="RBID">ISTEX:719EBEC207775099DCD192D8FF5FDF90F8CCE622</idno>
<date when="2009" year="2009">2009</date>
<idno type="doi">10.1111/j.1365-2966.2009.15560.x</idno>
<idno type="url">https://api.istex.fr/document/719EBEC207775099DCD192D8FF5FDF90F8CCE622/fulltext/pdf</idno>
<idno type="wicri:Area/Main/Corpus">000772</idno>
<idno type="wicri:Area/Main/Curation">000772</idno>
<idno type="wicri:Area/Main/Exploration">000128</idno>
<idno type="wicri:explorRef" wicri:stream="Main" wicri:step="Exploration">000128</idno>
</publicationStmt>
<sourceDesc>
<biblStruct>
<analytic>
<title level="a" type="main" xml:lang="en">Modelling galaxy clustering: is new physics needed in galaxy formation models?</title>
<author>
<name sortKey="Kim, Han Eek" sort="Kim, Han Eek" uniqKey="Kim H" first="Han-Seek" last="Kim">Han-Seek Kim</name>
<affiliation>
<wicri:noCountry code="subField">3LE</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Baugh, C M" sort="Baugh, C M" uniqKey="Baugh C" first="C. M." last="Baugh">C. M. Baugh</name>
<affiliation>
<wicri:noCountry code="subField">3LE</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Cole, S" sort="Cole, S" uniqKey="Cole S" first="S." last="Cole">S. Cole</name>
<affiliation>
<wicri:noCountry code="subField">3LE</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Frenk, C S" sort="Frenk, C S" uniqKey="Frenk C" first="C. S." last="Frenk">C. S. Frenk</name>
<affiliation>
<wicri:noCountry code="subField">3LE</wicri:noCountry>
</affiliation>
</author>
<author>
<name sortKey="Benson, A J" sort="Benson, A J" uniqKey="Benson A" first="A. J." last="Benson">A. J. Benson</name>
<affiliation wicri:level="1">
<country xml:lang="fr">États-Unis</country>
<wicri:regionArea>Theoretical Astrophysics, Caltech, MC350‐17, 1200 E. California Blvd, 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 Publishing Ltd</publisher>
<pubPlace>Oxford, UK</pubPlace>
<date type="published" when="2009-12-11">2009-12-11</date>
<biblScope unit="volume">400</biblScope>
<biblScope unit="issue">3</biblScope>
<biblScope unit="page" from="1527">1527</biblScope>
<biblScope unit="page" to="1540">1540</biblScope>
</imprint>
<idno type="ISSN">0035-8711</idno>
</series>
<idno type="istex">719EBEC207775099DCD192D8FF5FDF90F8CCE622</idno>
<idno type="DOI">10.1111/j.1365-2966.2009.15560.x</idno>
<idno type="ArticleID">MNR15560</idno>
</biblStruct>
</sourceDesc>
<seriesStmt>
<idno type="ISSN">0035-8711</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>galaxies: formation</term>
<term>galaxies: interactions</term>
<term>large‐scale structure of Universe</term>
</keywords>
</textClass>
<langUsage>
<language ident="en">en</language>
</langUsage>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">The clustering amplitude of galaxies depends on their intrinsic luminosity. We compare the properties of publicly available galaxy formation models with clustering measurements from the Two‐degree Field Galaxy Redshift Survey. The model predictions show the same qualitative behaviour as the data but fail to match the observations at the level of accuracy at which current measurements can be made. We demonstrate that this is due to the model producing too many satellite galaxies in massive haloes. We implement simple models to describe two new processes: satellite–satellite mergers and the tidal dissolution of satellites to investigate their impact on the predicted clustering. We find that both processes need to be included in order to produce a model which matches the observations.</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>États-Unis</li>
</country>
</list>
<tree>
<noCountry>
<name sortKey="Baugh, C M" sort="Baugh, C M" uniqKey="Baugh C" first="C. M." last="Baugh">C. M. Baugh</name>
<name sortKey="Cole, S" sort="Cole, S" uniqKey="Cole S" first="S." last="Cole">S. Cole</name>
<name sortKey="Frenk, C S" sort="Frenk, C S" uniqKey="Frenk C" first="C. S." last="Frenk">C. S. Frenk</name>
<name sortKey="Kim, Han Eek" sort="Kim, Han Eek" uniqKey="Kim H" first="Han-Seek" last="Kim">Han-Seek Kim</name>
</noCountry>
<country name="États-Unis">
<noRegion>
<name sortKey="Benson, A J" sort="Benson, A J" uniqKey="Benson A" first="A. J." last="Benson">A. J. Benson</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 000128 | SxmlIndent | more

Ou

HfdSelect -h $EXPLOR_AREA/Data/Main/Exploration/biblio.hfd -nk 000128 | 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:719EBEC207775099DCD192D8FF5FDF90F8CCE622
   |texte=   Modelling galaxy clustering: is new physics needed in galaxy formation models?
}}

Wicri

This area was generated with Dilib version V0.6.32.
Data generation: Sat Nov 11 11:37:59 2017. Site generation: Mon Feb 12 16:27:53 2024