Interpreting the complex line profiles in the stellar spectra

Details Interpreting the complex line profiles in the stellar spectra Interpreting the complex line profiles in the stellar spectra

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009newar..53..214d&link_type=abstract

New Astronomy Reviews, Volume 53, Issue 7-10, p. 214-221.

Astronomy and Astrophysics

Astronomy

2

Scientific paper

In this review we present our recent investigation of the complex absorption lines in spectra of hot emission stars. The lines are created in a material ejected from stars (here we call it density regions around the objects). Particularly we present a model (GR model) which is developed to study satellite or discrete absorption components (SACs or DACs). Using the model we are able to extract kinematical parameters (rotational, radial and random velocity) and some physical parameters (full width at half maximum, optical depth in the center of the line, column density and absorbed or emitted energy) of the density regions.

Affiliated with

Also associated with

No associations

Rating

Interpreting the complex line profiles in the stellar spectra 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 Interpreting the complex line profiles in the stellar spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interpreting the complex line profiles in the stellar spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-766690