Ultraviolet Line Profiles of AGN -- Cycle 1

Details Ultraviolet Line Profiles of AGN -- Cycle 1 Ultraviolet Line Profiles of AGN -- Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.3211b&link_type=abstract

HST Proposal ID #3211

Computer Science

Hst Proposal Id #3211

Scientific paper

We will observe various emission lines in the Seyfert galaxy NGC 7469. These data will be compared to optical emission lines to look for line profile differences that would indicate spatial and ionization stratification within the broad-line region. Line ratios will also yield information about the photoionization conditions in the BLR. NGC 7469 is of interest since Hbeta has a strong red asymmetry which is uncommon in Seyfert galaxies.

Affiliated with

Also associated with

No associations

Rating

Ultraviolet Line Profiles of AGN -- Cycle 1 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 Ultraviolet Line Profiles of AGN -- Cycle 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultraviolet Line Profiles of AGN -- Cycle 1 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-862604