Line emission and absorption characteristics due to stellar winds in active galactic nuclei.

Details Line emission and absorption characteristics due to stellar winds in active galactic nuclei. Line emission and absorption characteristics due to stellar winds in active galactic nuclei.

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997baas...29..846t&link_type=gif

Bulletin of the Astronomical Society, Vol. 29, No. 2, p. 846

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei: Stellar Winds, Active Galactic Nuclei: Emission Lines, Active Galactic Nuclei: Absorption Lines

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

Line emission and absorption characteristics due to stellar winds in active galactic nuclei. 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 Line emission and absorption characteristics due to stellar winds in active galactic nuclei., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Line emission and absorption characteristics due to stellar winds in active galactic nuclei. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-836549