Double-peaked Narrow Emission Lines In AGN: Jets, Spins Or Twins?

Details Double-peaked Narrow Emission Lines In AGN: Jets, Spins Or Twins? Double-peaked Narrow Emission Lines In AGN: Jets, Spins Or Twins?

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21714258s&link_type=abstract

American Astronomical Society, AAS Meeting #217, #142.58; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

AGN with double-peaked narrow lines have attracted recent attention as candidates for binary AGN in galaxy mergers. However, double-peaked lines can also result from bipolar jets or rotating disks. We examine tests of these possibilities involving the properties of the emission lines. Indicators based on the velocity separation of the components suggest that objects with equal intensity peaks may be rotating disks.

Affiliated with

Also associated with

No associations

Rating

Double-peaked Narrow Emission Lines In AGN: Jets, Spins Or Twins? 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 Double-peaked Narrow Emission Lines In AGN: Jets, Spins Or Twins?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Double-peaked Narrow Emission Lines In AGN: Jets, Spins Or Twins? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1394402