近距离银河系星系的多波段研究
摘要
One of the least biased complete Seyfert sample available to date has been considered to perform an X-ray survey using the capabilities of XMM-Newton and Chandra satellites. The X-ray nuclear luminosities obtained have been used to perform a multi-wavelength analysis as a powerfull tool in the identification of heavily obscured objects. The new X-ray data, together with highest quality nuclear fluxes available from the radio to the optical band, allow us to obtain nuclear Spectral Energy Distributions (SEDs) for type 1 and type 2 objects in our sample. The results obtained from the analysis of the SED have been discussed in the framework of Unified Models.
引用
@article{arxiv.astro-ph/0410083,
title = {Multi-wavelength study of a sample of nearby Seyfert galaxies},
author = {F. Panessa and L. Bassani and M. Cappi and M. Dadina and K. Iwasawa},
journal= {arXiv preprint arXiv:astro-ph/0410083},
year = {2007}
}
备注
8 pages, 8 figures. Proceedings of the VI Italian Conference on Active Galactic Nuclei. See http://www.arcetri.astro.it/~agn6/proceedings/