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1. Identity statement
Reference TypeJournal Article
Sitemtc-m16c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier6qtX3pFwXQZ3P8SECKy/EtTmr
Repositorysid.inpe.br/jeferson/2004/12.16.11.08
Last Update2006:06.14.04.18.50 (UTC) administrator
Metadata Repositorysid.inpe.br/jeferson/2004/12.16.11.08.09
Metadata Last Update2018:06.04.04.12.58 (UTC) administrator
Secondary KeyINPE-12557-PRE/7854
ISBN/ISSN0035-8711
ISSN1365-2966
Citation KeyFernandesCarvContGal:2004:MaStPo
TitleMassive star populations in wolf-rayet galaxies
Year2004
MonthDec.
Access Date2024, May 16
Secondary TypePRE PI
Number of Files1
Size459 KiB
2. Context
Author1 Fernandes, I. F
2 Carvalho, Reinaldo Ramos de
3 Contini, T
4 Gal, R. R.
Resume Identifier1
2 8JMKD3MGP5W/3C9JJ5B
Group1 DAS-INPE-MCT-BR
Affiliation1 Univ Sao Paulo, Inst Astron & Geofis, Sao Paulo
2 Instituto Nacional de Pesquisas Espaciais,Divisão de Astrofisica(INPE,DAS)
3 Observ Midi Pyrenees, Astrophys Lab, UMR 5572, Toulouse, F-31400 France
4 Univ Calif Davis, Dept Phys, Davis, CA 95616 USA
JournalMonthly Notices of the Royal Astronomical Society
Volume355
Number3
Pages728-746
History (UTC)2004-12-16 13:08:10 :: alexandra -> marciana ::
2005-06-14 17:04:36 :: marciana -> administrator ::
2006-09-27 21:01:24 :: administrator -> marciana ::
2008-05-02 16:20:27 :: marciana -> administrator ::
2018-06-04 04:12:58 :: administrator -> marciana :: 2004
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Keywordsgalaxies : abundances
galaxies : evolution
galaxies : starburst /H-II-REGIONS
EMISSION-LINE GALAXIES
PRIMORDIAL HELIUM ABUNDANCE
LONG-SLIT SPECTROSCOPY
BARRED SPIRAL GALAXIES
GALACTIC HII-REGIONS
STARBURST GALAXIES
CHEMICAL ABUNDANCES
GASEOUS NEBULAE
IONIZED-GAS
AbstractWe analyse long-slit spectral observations of 14 Wolf-Rayet (WR) galaxies from the sample of Schaerer, Contini & Pindao. All 14 galaxies show broad WR emission in the blue region of the spectrum, consisting of a blend of IIIlambda4640,CIIIlambda4650, CIVlambda4658 and HeIIlambda4686 emission lines, which is a spectral characteristic of WN stars. Broad CIVlambda5808 emission, termed the red bump, is detected in nine galaxies and CIIIlambda5996 is detected in six galaxies. These emission features are due to WC stars. We derive the numbers of late WN and early WC stars from the luminosity of the blue and red bumps, respectively. The number of O stars is estimated from the luminosity of the Hbeta emission line, after subtracting the contribution of WR stars. The Schaerer & Vacca models predict that the number of WR stars relative to O stars, N-WR/N-O, increases with metallicity. For low-metallicity galaxies, the results agree with predictions of evolutionary synthesis models for galaxies with a burst of star formation, and indicate an initial mass function (IMF) slope -2 less than or similar to Gamma less than or similar to -2.35 in the low-metallicity regime. For high-metallicity galaxies our observations suggest a Salpeter IMF (Gamma = -2.35) and an extended short burst. The main possible sources of error are the adopted luminosities for single WCE and WNL stars. We also report, for the first time, on NGC 450 as a galaxy with WR characteristics. For NGC 450, we estimate the number of WN and WC stars. The number ratio N-WR/N-O, and the equivalent widths of the blue bump, EWlambda4686, and of the red bump, EWlambda5808, in NGC 450 are also in good agreement with the instantaneous burst model prediction for WR galaxies.
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > Massive star populations...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Contentthere are no files
4. Conditions of access and use
data URLhttp://urlib.net/ibi/6qtX3pFwXQZ3P8SECKy/EtTmr
zipped data URLhttp://urlib.net/zip/6qtX3pFwXQZ3P8SECKy/EtTmr
Languageen
Target Filemassive.pdf
User Groupadministrator
alexandra
marciana
Visibilityshown
Copy HolderSID/SCD
Archiving Policyallowpublisher allowfinaldraft
Read Permissionallow from all
5. Allied materials
Next Higher Units8JMKD3MGPCW/3ETR8EH
DisseminationWEBSCI; PORTALCAPES; MGA; COMPENDEX.
Host Collectionsid.inpe.br/mtc-m18@80/2008/03.17.15.17
6. Notes
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