Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203
Autor(a) principal: | |
---|---|
Data de Publicação: | 2003 |
Outros Autores: | |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Institucional da UFRGS |
Texto Completo: | http://hdl.handle.net/10183/206302 |
Resumo: | We investigate the stellar population content in the lenticular galaxies NGC1023, NGC3115 and NGC4203 applying a population synthesis method based on a seven component spectral basis with different ages – 2.5 × 106, 10× 106, 25× 106, 75× 106, 200 × 106,1 .2 × 109 and older than 1010 years, and metallicity in the range −1.3 ≤ [Z/Z ] ≤− 0.2. This study employs two-dimensional STIS spectra in the range λλ2900–5700 Å, obtained from the Hubble Space Telescope public archives. We extracted one-dimensional spectra in adjacent windows 100 pc wide (projected distance) from the nuclear regions up to 300–400 pc. The largest contribution, both in λ5870Å flux and mass fraction, comes from old stars (age > 1010 years). We verified the possible existence of circumnuclear bursts (CNBs) in NGC3115 and NGC4203. |
id |
UFRGS-2_d9d6fc14b76be7ef146b81168c3f7125 |
---|---|
oai_identifier_str |
oai:www.lume.ufrgs.br:10183/206302 |
network_acronym_str |
UFRGS-2 |
network_name_str |
Repositório Institucional da UFRGS |
repository_id_str |
|
spelling |
Bassin Filho, MáximoBonatto, Charles Jose2020-02-28T04:05:50Z20030004-6361http://hdl.handle.net/10183/206302000387754We investigate the stellar population content in the lenticular galaxies NGC1023, NGC3115 and NGC4203 applying a population synthesis method based on a seven component spectral basis with different ages – 2.5 × 106, 10× 106, 25× 106, 75× 106, 200 × 106,1 .2 × 109 and older than 1010 years, and metallicity in the range −1.3 ≤ [Z/Z ] ≤− 0.2. This study employs two-dimensional STIS spectra in the range λλ2900–5700 Å, obtained from the Hubble Space Telescope public archives. We extracted one-dimensional spectra in adjacent windows 100 pc wide (projected distance) from the nuclear regions up to 300–400 pc. The largest contribution, both in λ5870Å flux and mass fraction, comes from old stars (age > 1010 years). We verified the possible existence of circumnuclear bursts (CNBs) in NGC3115 and NGC4203.application/pdfengAstronomy and astrophysics. Les Ulis. Vol. 410, no. 3 (Nov. 2003), p. 803-812Nucleo galaticoGaláxiasPopulacoes estelaresGalaxies: elliptical and lenticular, cDGalaxies: stellar contentGalaxies: nucleiStellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203Estrangeiroinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/openAccessreponame:Repositório Institucional da UFRGSinstname:Universidade Federal do Rio Grande do Sul (UFRGS)instacron:UFRGSTEXT000387754.pdf.txt000387754.pdf.txtExtracted Texttext/plain38688http://www.lume.ufrgs.br/bitstream/10183/206302/2/000387754.pdf.txt9762505f119663e4b2294c788d5f3b71MD52ORIGINAL000387754.pdfTexto completo (inglês)application/pdf552021http://www.lume.ufrgs.br/bitstream/10183/206302/1/000387754.pdf07de641204e694a009cd008b28cdc5a4MD5110183/2063022023-07-15 03:27:18.666634oai:www.lume.ufrgs.br:10183/206302Repositório de PublicaçõesPUBhttps://lume.ufrgs.br/oai/requestopendoar:2023-07-15T06:27:18Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS)false |
dc.title.pt_BR.fl_str_mv |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 |
title |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 |
spellingShingle |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 Bassin Filho, Máximo Nucleo galatico Galáxias Populacoes estelares Galaxies: elliptical and lenticular, cD Galaxies: stellar content Galaxies: nuclei |
title_short |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 |
title_full |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 |
title_fullStr |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 |
title_full_unstemmed |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 |
title_sort |
Stellar population gradient in lenticular galaxies : NGC 1023, NGC 3115 and NGC 4203 |
author |
Bassin Filho, Máximo |
author_facet |
Bassin Filho, Máximo Bonatto, Charles Jose |
author_role |
author |
author2 |
Bonatto, Charles Jose |
author2_role |
author |
dc.contributor.author.fl_str_mv |
Bassin Filho, Máximo Bonatto, Charles Jose |
dc.subject.por.fl_str_mv |
Nucleo galatico Galáxias Populacoes estelares |
topic |
Nucleo galatico Galáxias Populacoes estelares Galaxies: elliptical and lenticular, cD Galaxies: stellar content Galaxies: nuclei |
dc.subject.eng.fl_str_mv |
Galaxies: elliptical and lenticular, cD Galaxies: stellar content Galaxies: nuclei |
description |
We investigate the stellar population content in the lenticular galaxies NGC1023, NGC3115 and NGC4203 applying a population synthesis method based on a seven component spectral basis with different ages – 2.5 × 106, 10× 106, 25× 106, 75× 106, 200 × 106,1 .2 × 109 and older than 1010 years, and metallicity in the range −1.3 ≤ [Z/Z ] ≤− 0.2. This study employs two-dimensional STIS spectra in the range λλ2900–5700 Å, obtained from the Hubble Space Telescope public archives. We extracted one-dimensional spectra in adjacent windows 100 pc wide (projected distance) from the nuclear regions up to 300–400 pc. The largest contribution, both in λ5870Å flux and mass fraction, comes from old stars (age > 1010 years). We verified the possible existence of circumnuclear bursts (CNBs) in NGC3115 and NGC4203. |
publishDate |
2003 |
dc.date.issued.fl_str_mv |
2003 |
dc.date.accessioned.fl_str_mv |
2020-02-28T04:05:50Z |
dc.type.driver.fl_str_mv |
Estrangeiro info:eu-repo/semantics/article |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10183/206302 |
dc.identifier.issn.pt_BR.fl_str_mv |
0004-6361 |
dc.identifier.nrb.pt_BR.fl_str_mv |
000387754 |
identifier_str_mv |
0004-6361 000387754 |
url |
http://hdl.handle.net/10183/206302 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.ispartof.pt_BR.fl_str_mv |
Astronomy and astrophysics. Les Ulis. Vol. 410, no. 3 (Nov. 2003), p. 803-812 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.source.none.fl_str_mv |
reponame:Repositório Institucional da UFRGS instname:Universidade Federal do Rio Grande do Sul (UFRGS) instacron:UFRGS |
instname_str |
Universidade Federal do Rio Grande do Sul (UFRGS) |
instacron_str |
UFRGS |
institution |
UFRGS |
reponame_str |
Repositório Institucional da UFRGS |
collection |
Repositório Institucional da UFRGS |
bitstream.url.fl_str_mv |
http://www.lume.ufrgs.br/bitstream/10183/206302/2/000387754.pdf.txt http://www.lume.ufrgs.br/bitstream/10183/206302/1/000387754.pdf |
bitstream.checksum.fl_str_mv |
9762505f119663e4b2294c788d5f3b71 07de641204e694a009cd008b28cdc5a4 |
bitstream.checksumAlgorithm.fl_str_mv |
MD5 MD5 |
repository.name.fl_str_mv |
Repositório Institucional da UFRGS - Universidade Federal do Rio Grande do Sul (UFRGS) |
repository.mail.fl_str_mv |
|
_version_ |
1801224987106869248 |