Line formation calculation for an expanding stellar atmosphere using the linearized separation method.

Details Line formation calculation for an expanding stellar atmosphere using the linearized separation method. Line formation calculation for an expanding stellar atmosphere using the linearized separation method.

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..163w&link_type=abstract

Acta Astrophys. Sin., Vol. 15, No. 2, p. 163 - 173

Astronomy and Astrophysics

Astrophysics

2

Stellar Atmospheres: Line Formation, Stellar Atmospheres: Radiative Transfer, Stellar Atmospheres: P Cygni Profiles

Scientific paper

Having carefully investigated the radiative transfer process in stellar atmospheres with extended outflowing envelopes, the authors present a new non-LTE atmosphere code to calculate line profiles in such stars. The line transfer is treated using the linearized separation method, which may both save computing time and have quick convergency. The authors use this method to analyse the Hα P Cygni profile of ɛ Ori and get good agreement between theoretical and observational profiles.

Affiliated with

Also associated with

No associations

Rating

Line formation calculation for an expanding stellar atmosphere using the linearized separation method. 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 formation calculation for an expanding stellar atmosphere using the linearized separation method., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Line formation calculation for an expanding stellar atmosphere using the linearized separation method. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1827325