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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16b.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZGivnK2Y/QesR2
Repositorysid.inpe.br/mtc-m17@80/2007/05.23.19.05   (restricted access)
Last Update2007:05.23.19.05.06 (UTC) administrator
Metadata Repositorysid.inpe.br/mtc-m17@80/2007/05.23.19.05.08
Metadata Last Update2018:06.05.03.34.09 (UTC) administrator
Secondary KeyINPE--PRE/
ISSN0004-6256
Citation KeyLaRosaCarvVazdBarb:2007:StPoSt
TitleTruncated star formation in compact groups of galaxies: a stellar population study
Year2007
MonthJan.
Access Date2024, Apr. 28
Secondary TypePRE PI
Number of Files1
Size442 KiB
2. Context
Author1 De La Rosa, I. G.
2 Carvalho, Reinaldo Roberto de
3 Vazdekis, A.
4 Barbuy, B.
Group1
2 DAS-INPE-MCT-BR
Affiliation1 Instituto de Astrofisica de Canarias
2 Instituto Nacional de Pesquisas Espaciais (INPE)
3 Instituto de Astrofisica de Canarias
4 Universidade de São Paulo. Instituto Astronômico e Geofísico (USP. IAG)
JournalAstronomical Journal
Volume133
Pages330-346
History (UTC)2007-07-10 14:24:10 :: simone -> administrator ::
2010-05-11 02:08:26 :: administrator -> simone ::
2010-05-18 13:12:35 :: simone -> administrator ::
2012-10-23 23:52:48 :: administrator -> simone :: 2007
2013-02-20 15:19:57 :: simone -> administrator :: 2007
2018-06-05 03:34:09 :: administrator -> marciana :: 2007
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
KeywordsGalaxies: clusters: general
Galaxies: evolution
Galaxies: interactions
ASTROPHYSICS
AbstractWe present the results of a study comparing the stellar populations in the elliptical galaxies of Hickson compact groups (HCGs) with those in low-density environments. We analyze a sample of intermediate-resolution (4.25 8 FWHM) spectra of 22 galaxies in HCGs and 12 in the field or in loose groups. Three different population-synthesis models and stellar population analyses are used to make the results more robust. Great care has been taken to correct for the emission contamination of the Balmer lines, used to determine the mean luminosity-weighted ages of the galaxies.We find that, on average, galaxies in HCGs are systematically older and more metal-poor than in the field, in agreement with previous works. The most interesting finding is that the low- galaxies in HCGs show an enhanced [Mg/Fe] ratio and depleted metallicity [Z/H] with respect to their counterparts in the field. This anomalous behavior is interpreted as evidence for the action of a mechanism that truncates the star formation (SF). Hydrodynamic simulations of galaxy mergers (Di Matteo et al. 2005) support this interpretation by predicting the quenching of SF soon after the merger event. Combining this scenario and the evidence presented here, the HCGs, generally considered to be ideal environments for galaxy-galaxy interactions, become ideal places for SF truncation.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Truncated star formation...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
Target FileTruncated_La%20Rosa.pdf
User Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft
Read Permissiondeny from all and allow from 150.163
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES.
Host Collectionlcp.inpe.br/ignes/2004/02.12.18.39
cptec.inpe.br/walmeida/2003/04.25.17.12
6. Notes
Empty Fieldsalternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel documentstage doi e-mailaddress electronicmailaddress format isbn label lineage mark mirrorrepository nextedition notes number orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup resumeid rightsholder schedulinginformation secondarydate secondarymark session shorttitle sponsor subject tertiarymark tertiarytype typeofwork url versiontype
7. Description control
e-Mail (login)marciana
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