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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3ARNGDB
Repositorydpi.inpe.br/plutao/2011/11.23.18.51   (restricted access)
Last Update2011:12.08.11.51.26 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2011/11.23.18.51.01
Metadata Last Update2018:06.05.00.01.37 (UTC) administrator
DOI10.1088/2041-8205/740/2/L41
ISSN2041-8205
2041-8213
Labellattes: 7418724825594141 3 BarberaFeCaLoPaLaLu:2011:RASTCO
Citation KeyBarberaFeCaLoPaLaLu:2011:RaStCo
TitleOn the radial stellar content of early-type galaxies as a function of mass and environment
Year2011
MonthOct
Access Date2024, May 05
Secondary TypePRE PI
Number of Files1
Size188 KiB
2. Context
Author1 Barbera, F. La
2 Ferreras, I.
3 de Carvalho, Reinaldo Ramos
4 Lopes, Paulo Afrânio Augusto
5 Pasquali, A.
6 De La Rosa, I. G.
7 De Lucia, G.
Resume Identifier1
2
3 8JMKD3MGP5W/3C9JJ5B
Group1
2
3 DAS-CEA-INPE-MCT-BR
4 DAS-CEA-INPE-MCT-BR
Affiliation1
2
3 Instituto Nacional de Pesquisas Espaciais (INPE)
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3 rrdecarvalho2008@gmail.com
e-Mail Addressrrdecarvalho2008@gmail.com
JournalAstrophysical Journal Letters
Volume740
Number2
PagesL41
History (UTC)2011-11-24 11:03:16 :: lattes -> secretaria.cpa@dir.inpe.br :: 2011
2011-12-08 11:51:40 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2018-06-05 00:01:37 :: administrator -> marciana :: 2011
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsGalaxies: Clusters: general
Galaxies: Evolution
Galaxies: fundamental parameters
AbstractUsing optical-optical and optical-NIR colors, we analyze the radial dependence of age and metallicity inside massive (M(star) greater than or similar to 10(10.5) M(circle dot)), low-redshift (z < 0.1), early-type galaxies (ETGs), residing in both high-density group regions and the field. On average, internal color gradients of ETGs are mainly driven by metallicity, consistent with previous studies. However, we find that group galaxies feature positive age gradients, del(t), i.e., a younger stellar population in the galaxy center, and steeper metallicity gradients, compared to the field sample, whose del(t) ranges from negative in lower mass galaxies to positive gradients at higher mass. These dependencies yield new constraints on models of galaxy formation and evolution. We speculate that age and metallicity gradients of group ETGs result from (either gas-rich or minor-dry) mergers and/or cold-gas accretion, while field ETGs exhibit the characteristic flatter gradients expected from younger, more metal-rich stars formed inside-out by later gas cooling.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > On the radial...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
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Languagept
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Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
Host Collectiondpi.inpe.br/plutao@80/2008/08.19.15.01
6. Notes
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