| 1. Identificação | ||||
| Tipo de Referência | Artigo em Revista Científica (Journal Article) | |||
| Site | mtc-m21b.sid.inpe.br | |||
| Código do Detentor | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identificador | 8JMKD3MGP3W34P/3HPC77H | |||
| Repositório | sid.inpe.br/mtc-m21b/2015/01.14.15.43 | |||
| Última Atualização | 2015:01.14.15.43.11 (UTC) administrator | |||
| Repositório de Metadados | sid.inpe.br/mtc-m21b/2015/01.14.15.43.11 | |||
| Última Atualização dos Metadados | 2018:06.04.02.55.13 (UTC) administrator | |||
| DOI | 10.1051/0004-6361/201424821 | |||
| ISSN | 0004-6361 1432-0746 | |||
| Chave de Citação | LaganáLoMaLaCaSc:2015:MeElSt | |||
| Título | A metal-rich elongated structure in the core of the group NGC 4325  | |||
| Ano | 2015 | |||
| Data de Acesso | 09 maio 2024 | |||
| Tipo de Trabalho | journal article | |||
| Tipo Secundário | PRE PI | |||
| Número de Arquivos | 1 | |||
| Tamanho | 2003 KiB | |||
| 2. Contextualização | ||||
| Autor | 1 Laganá, T. F. 2 Lovisari, L. 3 Martins, L. 4 Lanfranchi, G. A. 5 Capelato, Hugo Vicente 6 Schellenberger, G. | |||
| Identificador de Curriculo | 1 2 3 4 5 8JMKD3MGP5W/3C9JHCT | |||
| Grupo | 1 2 3 4 5 DAS-CEA-INPE-MCTI-GOV-BR | |||
| Afiliação | 1 Universidade Cruzeiro do Sul 2 Universität Bonn 3 Universidade Cruzeiro do Sul 4 Universidade Cruzeiro do Sul 5 Instituto Nacional de Pesquisas Espaciais (INPE) 6 Universität Bonn | |||
| Endereço de e-Mail do Autor | 1 tflagana@gmail.com 2 3 4 5 hugo@das.inpe.br | |||
| Revista | Astronomy & Astrophysics | |||
| Volume | 573 | |||
| Nota Secundária | A1_ENGENHARIAS_III A1_GEOCIÊNCIAS A2_INTERDISCIPLINAR A2_MATEMÁTICA_/_PROBABILIDADE_E A2_ENGENHARIAS_IV A2_ASTRONOMIA_/_FÍSICA B2_ENSINO C_ENGENHARIAS_II | |||
| Histórico (UTC) | 2015-01-14 15:44:15 :: simone -> administrator :: 2015 2018-06-04 02:55:13 :: administrator -> simone :: 2015 | |||
| 3. Conteúdo e estrutura | ||||
| É a matriz ou uma cópia? | é a matriz | |||
| Estágio do Conteúdo | concluido | |||
| Transferível | 1 | |||
| Tipo do Conteúdo | External Contribution | |||
| Tipo de Versão | publisher | |||
| Palavras-Chave | galaxies NGC 4325 intergalactic medium halos | |||
| Resumo | Aims. Based on XMM-Newton, Chandra, and optical DR10-SDSS data, we investigate the metal enrichment history of the group NGC 4325 (z = 0.026). To complete the analysis we used chemical evolution models and studied the optical spectrum of the central dominant galaxy through its stellar population analysis and emission line diagnostics to analyse its role in the metal enrichment of the intra-group medium. Methods. We used X-ray 2D spectrally resolved maps to resolve structure in temperature and metallicity. We also derived gas and total masses within r2500 and r500 assuming hydrostatic equilibrium and spherical symmetry. To perform stellar population analysis we applied the spectral fitting technique with STARLIGHT to the optical spectrum of the central galaxy. We simulated the chemical evolution of the central galaxy. Results. While the temperature, pseudo-pressure, and pseudo-entropy maps showed no inhomogeneities, the spatial distribution of the metallicity shows a filamentary structure in the core of this group, which is spatially correlated with the central galaxy, suggesting a connection between the two. The analysis of the optical spectrum of the central galaxy showed no contribution by any recent AGN activity. Using the star formation history as input to chemical evolution models, we predicted the iron and oxygen mass released by supernovae (SNe) winds in the central galaxy up to the present time. Conclusions. Comparing the predicted amount of mass released by the NGC 4325 galaxy to the ones derived through X-ray analysis we conclude that the winds from the central galaxy alone play a minor role in the IGM metal enrichment of this group inside r2500. The SNe winds are responsible for no more than 3% of it and of the iron mass and 21% of the oxygen mass enclosed within r2500. Our results suggest that oxygen has been produced in the early stages of the group formation, becoming well mixed and leading to an almost flat profile. Instead, the iron distribution is centrally peaked, indicating that this element is still being added to the IGM specifically in the core by the SNIa. A possible scenario to explain the elongated metal-rich structure in the core of the NGC 4325 is a past AGN activity, in which our results suggest an episode older than ~107−108 yrs and younger than 5 × 108. Through the overall distribution of the galaxies, we found no signs of recent merger in the group centre that could explain the metal-rich structure. | |||
| Área | CEA | |||
| Arranjo | urlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > A metal-rich elongated... | |||
| Conteúdo da Pasta doc | acessar | |||
| Conteúdo da Pasta source | não têm arquivos | |||
| Conteúdo da Pasta agreement |
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| 4. Condições de acesso e uso | ||||
| URL dos dados | http://urlib.net/ibi/8JMKD3MGP3W34P/3HPC77H | |||
| URL dos dados zipados | http://urlib.net/zip/8JMKD3MGP3W34P/3HPC77H | |||
| Idioma | en | |||
| Arquivo Alvo | metal rich.pdf | |||
| Grupo de Usuários | administrator simone | |||
| Grupo de Leitores | administrator simone | |||
| Visibilidade | shown | |||
| Política de Arquivamento | allowpublisher allowfinaldraft | |||
| Permissão de Leitura | allow from all | |||
| Permissão de Atualização | não transferida | |||
| 5. Fontes relacionadas | ||||
| Repositório Espelho | urlib.net/www/2011/03.29.20.55 | |||
| Unidades Imediatamente Superiores | 8JMKD3MGPCW/3ETR8EH | |||
| Lista de Itens Citando | sid.inpe.br/mtc-m21/2012/07.13.14.50.04 1 | |||
| Divulgação | WEBSCI; PORTALCAPES; COMPENDEX; SCOPUS. | |||
| Acervo Hospedeiro | sid.inpe.br/mtc-m21b/2013/09.26.14.25.20 | |||
| 6. Notas | ||||
| Campos Vazios | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark month nextedition notes number orcid pages parameterlist parentrepositories previousedition previouslowerunit progress project rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Controle da descrição | ||||
| e-Mail (login) | simone | |||
| atualizar | ||||