Similarity Between DACs/SACs Phenomena in Hot Emission Stars and Quasars Absorption Lines

Details Similarity Between DACs/SACs Phenomena in Hot Emission Stars and Quasars Absorption Lines Similarity Between DACs/SACs Phenomena in Hot Emission Stars and Quasars Absorption Lines

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1058..305d&link_type=abstract

SPECTRAL LINE SHAPES: Volume 15-19th International Conference on Spectral Line Shapes. AIP Conference Proceedings, Volume 1058,

Physics

Atomic Spectra, Late Stages Of Stellar Evolution, Quasars

Scientific paper

In the spectra of Hot Emission Stars and AGNs we observe some peculiar profiles that result from dynamical processes such as accretion and/or ejection of matter from these objects. In this paper we indicate that DACs and SACs phenomena, can explain the spectral lines peculiarity in Hot Emission Stars and AGNs. We also try to connect the physical properties of absorption regions around stars and quasars.

Affiliated with

Also associated with

No associations

Rating

Similarity Between DACs/SACs Phenomena in Hot Emission Stars and Quasars Absorption 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 Similarity Between DACs/SACs Phenomena in Hot Emission Stars and Quasars Absorption Lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Similarity Between DACs/SACs Phenomena in Hot Emission Stars and Quasars Absorption Lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1662826