X-ray spectra of Seyfert galaxies

dc.contributor.author	Ghosh, K. K
dc.contributor.author	Soundararajaperumal, S
dc.date.accessioned	2008-06-17T05:44:33Z
dc.date.available	2008-06-17T05:44:33Z
dc.date.issued	1992-11
dc.identifier.citation	MNRAS, Vol. 259, No. 1, pp. 175 - 190	en
dc.identifier.uri	http://hdl.handle.net/2248/2441
dc.description.abstract	A spectra analysis of eight Seyfert galaxies shows that while seven have soft excesses in their spectra, with no low-energy absorption, ESO 140-G43 exhibits low energy absorption, and may have weak soft excess that is hidden by its 10 exp 21/sq cm absorber. It is suggested that soft excesses are a common feature of Seyfert galaxies, and soft excess detection depends on low-energy absorption in the line-of-sight to the source. This and other results obtained suggest that the fluorescence from warm material can produce a high fluorescence yield for the Fe line	en
dc.format.extent	1685110 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Blackwell Publishing	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1992MNRAS.259..175G	en
dc.subject	ASTRONOMICAL SPECTROSCOPY	en
dc.subject	MARKARIAN GALAXIES	en
dc.subject	SEYFERT GALAXIES	en
dc.subject	X RAY SPECTRA	en
dc.subject	ABSORPTION SPECTRA	en
dc.subject	EMISSION SPECTRA	en
dc.subject	EXOSAT SATELLITE	en
dc.subject	GINGA SATELLITE	en
dc.subject	SPACEBORNE ASTRONOMY	en
dc.subject	SPECTRAL LINE WIDTH	en
dc.title	X-ray spectra of Seyfert galaxies	en
dc.type	Article	en