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1. Identity statement
Reference TypeJournal Article
Siteplutao.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
IdentifierJ8LNKAN8RW/3ARNGD7
Repositorydpi.inpe.br/plutao/2011/11.23.18.50.56   (restricted access)
Last Update2011:12.27.11.27.52 (UTC) administrator
Metadata Repositorydpi.inpe.br/plutao/2011/11.23.18.50.57
Metadata Last Update2021:07.28.22.06.41 (UTC) administrator
DOI10.1111/j.1745-3933.2011.01146.x
ISSN1745-3933
Labellattes: 7418724825594141 4 RosaLaBaFerrCarv:2011:LiThSt
Citation KeyRosaLaBaFerrCarv:2011:LiThSt
TitleThe link between the star formation history and [α/Fe]
Year2011
MonthSept
Access Date2024, May 05
Secondary TypePRE PI
Number of Files1
Size551 KiB
2. Context
Author1 Rosa, Ignacio G. de la
2 La Barbera, Francesco
3 Ferreras, Ignacio
4 Carvalho, Reinaldo Ramos de
Resume Identifier1
2
3
4 8JMKD3MGP5W/3C9JJ5B
Group1
2
3
4 DAS-CEA-INPE-MCT-BR
Affiliation1 Instituto de Astrofísica de Canarias
2 INAF – Osservatorio Astronomico di Capodimonte
3 Mullard Space Science Laboratory, University College London
4 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4 rrdecarvalho2008@gmail.com
e-Mail Addressrrdecarvalho2008@gmail.com
JournalMonthly Notices of the Royal Astronomical Society Letters
Volume418
Number1
PagesL74-L78
History (UTC)2011-11-24 11:03:16 :: lattes -> secretaria.cpa@dir.inpe.br :: 2011
2012-01-17 13:18:04 :: secretaria.cpa@dir.inpe.br -> administrator :: 2011
2021-07-28 22:06:41 :: 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: elliptical and lenticular
cD
galaxies: evolution
galaxies: formation
galaxies: stellar content
galaxies: structure
AbstractThe abundance ratios between key elements such as iron and -process elements carry a wealth of information on the star formation history (SFH) of galaxies. So far, simple chemical evolution models have linked [/Fe ] with the SFH time-scale, correlating large abundance ratios with short-lived SFH. The incorporation of full spectral fitting to the analysis of stellar populations allows for a more quantitative constraint between [/Fe ] and the SFH. In this letter, we provide, for the first time, an empirical correlation between [/Fe ] (measured from spectral indices) and the SFH (determined via a non-parametric spectral-fitting method). We offer an empirical version of the iconic outline of Thomas et al., relating star formation time-scale with galaxy mass, although our results suggest, in contrast, a significant population of old (≳10 Gyr) stars even for the lowest mass ellipticals (M/dyn ¡­ 3 ¡¿ 1010 M¢Á). In addition, the abundance ratio is found to be strongly correlated with the time to build up the stellar component, showing that the highest [/Fe ] (≳+0.2) are attained by galaxies with the shortest half-mass formation time (≲2 Gyr), or equivalently, with the smallest (≲40 per cent) fraction of populations younger than 10 Gyr. These observational results support the standard hypothesis that star formation incorporates the Fe-enriched interstellar medium into stars, lowering the high abundance ratio of the old populations.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The link between...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
Languageen
User Groupadministrator
lattes
secretaria.cpa@dir.inpe.br
Visibilityshown
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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7. Description control
e-Mail (login)marciana
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