Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Oli L Dors"'
Autor:
Oli L Dors, M Valerdi, R A Riffel, R Riffel, M V Cardaci, G F Hägele, Mark Armah, M Revalski, S R Flury, P Freitas-Lemes, E B Amôres, A C Krabbe, L Binette, A Feltre, T Storchi-Bergmann
For the first time, the sulphur abundance relative to hydrogen (S/H) in the Narrow Line Regions of a sample of Seyfert 2 nuclei (Sy 2s) has been derived via direct estimation of the electron temperature. Narrow emission line intensities from the SDSS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::62662ea46eff9bdd9b62c8ec6b1c7058
Autor:
Mónica V. Cardaci, Rogemar A. Riffel, Anna Feltre, C. P. Aydar, Guillermo F. Hägele, Oli L. Dors, Mark Kojo Armah, Angela Krabbe, Rogério Riffel
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
For the first time, neon abundance has been derived in the narrow line region from a sample of Seyfert 2 nuclei. In view of this, we compiled from the literature fluxes of optical and infrared (IR) narrow emission lines for 35 Seyfert 2 nuclei in the
Autor:
Janaína C do Nascimento, Oli L Dors, Thaisa Storchi-Bergmann, Nícolas D Mallmann, Rogério Riffel, Gabriele S Ilha, Rogemar A Riffel, Sandro B Rembold, Alice Deconto-Machado, Luiz N da Costa, Mark Armah
We derive the metallicity (traced by the O/H abundance) of the narrow-line region (NLR) of 108 Seyfert galaxies as well as radial metallicity gradients along their galaxy discs and of these of a matched control sample of no active galaxies. In view o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a3cba7bcaa4433cf2097fa2f8a26b431
Publikováno v:
Proceedings of the International Astronomical Union. 15:168-169
Interactions and mergers between dwarf galaxies are mostly gas-rich and should be marked by an intense star formation activity. But these processes, which are expected to be common at earlier times, are very difficult to observe at low redshifts. To
Publikováno v:
Revista UniVap, Vol 19, Iss 34, Pp 53-57 (2013)
Revista Univap; Vol. 19 No. 34 (2013): Revista Univap online Edição Especial Simpósio de Física e Astronomia do Vale do Paraíba / ISSN 2237-1753; 53-57
Revista Univap; v. 19 n. 34 (2013): Revista Univap online Edição Especial Simpósio de Física e Astronomia do Vale do Paraíba / ISSN 2237-1753; 53-57
Revista UniVap
Universidade do Vale do Paraíba (Univap)
instacron:UNIVAP
Revista Univap; Vol. 19 No. 34 (2013): Revista Univap online Edição Especial Simpósio de Física e Astronomia do Vale do Paraíba / ISSN 2237-1753; 53-57
Revista Univap; v. 19 n. 34 (2013): Revista Univap online Edição Especial Simpósio de Física e Astronomia do Vale do Paraíba / ISSN 2237-1753; 53-57
Revista UniVap
Universidade do Vale do Paraíba (Univap)
instacron:UNIVAP
O acúmulo de massa, proveniente do processo de interação que forma as galáxias com anel polar, é um fator que favorece as condições necessárias para disparar atividades nucleares não térmicas. Esse fato fomentou a análise química de dez g
Autor:
Enrique Perez-Montero, Mónica V. Cardaci, Guillermo F. Hägele, Irapuan Rodrigues, Angela Krabbe, Rogemar A. Riffel, Oli L. Dors
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 422:252-260
We investigate the excitation mechanisms of near-infrared [Fe ii] and H2 emission lines observed in Active Galactic Nuclei (AGNs). We built a photoionization model grid considering a two-component continuum, one accounts for the Big Bump component pe
Aims: We derive the age and metallicity of circumnuclear star formation regions (CNSFRs) located in the spiral galaxies NGC6951 and NGC1097, and investigate the cause of the very low equivalent widths of emission lines found for these regions. Method
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::60485b2609715b883c39d5946dbdd537
http://arxiv.org/abs/0802.2070
http://arxiv.org/abs/0802.2070
We analyse two-dimensional near-IR K-band spectra from the inner 660x315 pc^2 of the Seyfert galaxy NGC7582 obtained with the Gemini GNIRS IFU. The nucleus harbors an unresolved source well reproduced by a blackbody of temperature T 1050 K, which we
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::151161f015dcd138966ebddccf347e1b
Autor:
Andrew Robinson, Kambiz Fathi, Rogemar A. Riffel, Oli L. Dors, Alessandro Marconi, David J. Axon, Thaisa Storchi-Bergmann, Göran Östlin
We report the discovery of gas streaming motions along nuclear spiral arms towards the LINER nucleus of the galaxy NGC 6951. The observations, obtained using the GMOS integral field spectrograph on the Gemini North telescope, yielded maps of the flux
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::aa837054c90da51b5e988c5c1014db51
http://arxiv.org/abs/0707.4176
http://arxiv.org/abs/0707.4176
Autor:
Jake S Bennett, Oli L. Dors, Ewald Puchwein, Linhua Jiang, Yucheng Guo, Nick Henden, Michele Ginolfi, Tohru Nagao, Debora Sijacki, Roberto Maiolino, Kenta Matsuoka
Publikováno v:
The Astrophysical Journal