1. Identity statement | |
Reference Type | Journal Article |
Site | plutao.sid.inpe.br |
Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S |
Identifier | J8LNKAN8RW/3ARNGD7 |
Repository | dpi.inpe.br/plutao/2011/11.23.18.50.56 (restricted access) |
Last Update | 2011:12.27.11.27.52 (UTC) administrator |
Metadata Repository | dpi.inpe.br/plutao/2011/11.23.18.50.57 |
Metadata Last Update | 2021:07.28.22.06.41 (UTC) administrator |
DOI | 10.1111/j.1745-3933.2011.01146.x |
ISSN | 1745-3933 |
Label | lattes: 7418724825594141 4 RosaLaBaFerrCarv:2011:LiThSt |
Citation Key | RosaLaBaFerrCarv:2011:LiThSt |
Title | The link between the star formation history and [α/Fe] |
Year | 2011 |
Month | Sept |
Access Date | 2024, May 05 |
Secondary Type | PRE PI |
Number of Files | 1 |
Size | 551 KiB |
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2. Context | |
Author | 1 Rosa, Ignacio G. de la 2 La Barbera, Francesco 3 Ferreras, Ignacio 4 Carvalho, Reinaldo Ramos de |
Resume Identifier | 1 2 3 4 8JMKD3MGP5W/3C9JJ5B |
Group | 1 2 3 4 DAS-CEA-INPE-MCT-BR |
Affiliation | 1 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 Address | 1 2 3 4 rrdecarvalho2008@gmail.com |
e-Mail Address | rrdecarvalho2008@gmail.com |
Journal | Monthly Notices of the Royal Astronomical Society Letters |
Volume | 418 |
Number | 1 |
Pages | L74-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 |
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3. Content and structure | |
Is the master or a copy? | is the master |
Content Stage | completed |
Transferable | 1 |
Content Type | External Contribution |
Version Type | publisher |
Keywords | galaxies: elliptical and lenticular cD galaxies: evolution galaxies: formation galaxies: stellar content galaxies: structure |
Abstract | The 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. |
Area | CEA |
Arrangement | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The link between... |
doc Directory Content | access |
source Directory Content | there are no files |
agreement Directory Content | there are no files |
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4. Conditions of access and use | |
Language | en |
User Group | administrator lattes secretaria.cpa@dir.inpe.br |
Visibility | shown |
Read Permission | deny from all and allow from 150.163 |
Update Permission | not transferred |
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5. Allied materials | |
Next Higher Units | 8JMKD3MGPCW/3ETR8EH |
Host Collection | dpi.inpe.br/plutao@80/2008/08.19.15.01 |
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6. Notes | |
Empty Fields | alternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel dissemination format isbn lineage mark mirrorrepository nextedition notes orcid parameterlist parentrepositories previousedition previouslowerunit progress project readergroup rightsholder schedulinginformation secondarydate secondarykey secondarymark session shorttitle sponsor subject targetfile tertiarymark tertiarytype typeofwork url |
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7. Description control | |
e-Mail (login) | marciana |
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