Hostname: page-component-848d4c4894-mwx4w Total loading time: 0 Render date: 2024-06-24T14:15:23.082Z Has data issue: false hasContentIssue false
  • English
  • Français

An XMM-Newton view of a small sample of Seyfert, 1 Galaxies

Published online by Cambridge University Press:  08 June 2011

M. V. Cardaci ,
G. F. Hagele ,
M. Santos-Lleó ,
Y. Krongold ,
A. I. Díaz  and
P. Rodriguez-Pascual
M. V. Cardaci
Affiliation:
Universidad Autónoma de Madrid, Cantoblanco, 28049-Madrid, Spain email: monica.cardaci@uam.es Facultad de Cs. Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque s/n, 1900 La Plata, Argentina
G. F. Hagele
Affiliation:
Universidad Autónoma de Madrid, Cantoblanco, 28049-Madrid, Spain email: monica.cardaci@uam.es Facultad de Cs. Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque s/n, 1900 La Plata, Argentina
M. Santos-Lleó
Affiliation:
XMM-Newton Science Operation Centre, ESAC, ESA, PO Box 50727, 28080 Madrid, Spain
Y. Krongold
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 70-264, 04510 México DF, México
A. I. Díaz
Affiliation:
Universidad Autónoma de Madrid, Cantoblanco, 28049-Madrid, Spain email: monica.cardaci@uam.es
P. Rodriguez-Pascual
Affiliation:
XMM-Newton Science Operation Centre, ESAC, ESA, PO Box 50727, 28080 Madrid, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a detailed analysis of all the X-ray data taken by the XMM-Newton satellite of a small sample of five Seyfert 1 galaxies: ESO 359-G19, HE 1143-1810, CTS A08.12, Mkn 110, and UGC 11763. Our aim is to characterize the different components of the material that print the absorption and emission features in the X-ray spectra of these objects. The continuum emission was studied through the EPIC spectra taking advantage of the spectral range of these cameras. The high resolution RGS spectra were analyzed in order to characterize the absorbing features and the emission line features that arise in the spectra of these sources.

Keywords

galaxies: activegalaxies: Seyfertgalaxies: individual (UGC 11763 ESO 359-G19, HE 1143-1810, CTS A08.12, Mkn 110)X-rays: galaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S274: Advances in Plasma Astrophysics , September 2010 , pp. 369 - 372
Copyright
Copyright © International Astronomical Union 2011

References

Cardaci, M. V., Santos-Lleó, M., Krongold, Y., Hägele, G. F., Díaz, A. I., & Rodríguez-Pascual, P. 2009, A&A, 432, 15Google Scholar
Krongold, Y., Nicastro, F., Brickhouse, N. S., Elvis, M., Liedahl, D. A. & Mathur, S. 2003, ApJ, 597, 832CrossRefGoogle Scholar
Piconcelli, E., Jimenez-Bailón, E., Guainazzi, M., Schartel, N., Rodríguez-Pascual, P. M. & Santos-Lleó, M. 2005, A&A, 432, 15Google Scholar