The Contribution of Disc Emission in Spectra of AGN: from X-ray to Optical Emission Lines

Details The Contribution of Disc Emission in Spectra of AGN: from X-ray to Optical Emission Lines The Contribution of Disc Emission in Spectra of AGN: from X-ray to Optical Emission Lines

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..50p&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 50-50"

Other

Scientific paper

The double peaked broad emission lines observed in some AGN are supposed to be emitted from an accretion disk. The fraction of AGN with broad emission lines is small (below 5%). On the other hand, the broad Fe K alpha line that indicates the accretion disk emission is detected in around 25% to 50% of AGN (see Guainazzi et al. 2006). Here we discuss the effects which can hide the disk emission in Fe K alpha as well as in low ionized optical lines of AGN. Moreover, we give some ways to estimate the disk emission even if the emission is hidden.

Affiliated with

Also associated with

No associations

Rating

The Contribution of Disc Emission in Spectra of AGN: from X-ray to Optical Emission Lines does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Contribution of Disc Emission in Spectra of AGN: from X-ray to Optical Emission Lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Contribution of Disc Emission in Spectra of AGN: from X-ray to Optical Emission Lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1812635