| Texto completo | |
| Autor(es): |
Martins, Lucimara P.
[1]
;
Riffel, Rogerio
[2]
;
Rodriguez-Ardila, Alberto
[3]
;
Gruenwald, Ruth
[4]
;
de Souza, Ronaldo
[4]
Número total de Autores: 5
|
| Afiliação do(s) autor(es): | [1] NAT Univ Cruzeiro Sul, BR-868 Sao Paulo - Brazil
[2] Univ Fed Rio Grande do Sul, IF, Dept Astron, BR-91501970 Porto Alegre, RS - Brazil
[3] Lab Nacl Astrofis MCT, BR-37501064 Itajuba, MG - Brazil
[4] Univ Sao Paulo, Inst Astron & Geofis, BR-1226 Sao Paulo - Brazil
Número total de Afiliações: 4
|
| Tipo de documento: | Artigo Científico |
| Fonte: | Monthly Notices of the Royal Astronomical Society; v. 406, n. 4, p. 2185-2192, AUG 21 2010. |
| Citações Web of Science: | 11 |
| Resumo | |
We performed stellar population synthesis on the nuclear and extended regions of NGC 1068 by means of near-infrared spectroscopy to disentangle their spectral energy distribution components. This is the first time that such a technique is applied to the whole 0.8-2.4 mu m wavelength interval in this galaxy. NGC 1068 is one of the nearest and probably the most studied Seyfert 2 galaxy, becoming an excellent laboratory to study the interaction between black holes, the jets that they can produce and the medium in which they propagate. Our main result is that traces of young stellar population are found at similar to 100 pc south of the nucleus. The contribution of a power-law continuum in the centre is about 25 per cent, which is expected if the light is scattered from a Seyfert 1 nucleus. We find peaks in the contribution of the featureless continuum about 100-150 pc from the nucleus on both sides. They might be associated with regions where the jet encounters dense clouds. Further support to this scenario is given by the peaks of hot dust distribution found around these same regions and the H(2) emission-line profile, leading us to propose that the peaks might be associated to regions where stars are being formed. Hot dust also has an important contribution to the nuclear region, reinforcing the idea of the presence of a dense, circumnuclear torus in this galaxy. Cold dust appears mostly in the south direction, which supports the view that the south-west emission is behind the plane of the galaxy and is extinguished very likely by dust in the plane. Intermediate-age stellar population contributes significantly to the continuum, especially in the inner 200 pc. (AU) | |
| Processo FAPESP: | 07/04316-1 - Traçadores de formação estelar no infravermelho |
| Beneficiário: | Lucimara Pires Martins |
| Modalidade de apoio: | Bolsas no Exterior - Pesquisa |