Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....80..138b&link_type=abstract
Astronomy and Astrophysics, vol. 80, no. 2, Dec. 1979, p. 138-146. Deutsche Forschungsgemeinschaft
Astronomy and Astrophysics
Astrophysics
23
Late Stars, Line Shape, Radiative Transfer, Stellar Envelopes, Stellar Spectra, Angular Momentum, Galactic Rotation, Line Spectra, Nebulae, Velocity Distribution
Scientific paper
A numerical method is presented which solves the line transfer problem in axisymmetric velocity fields and envelope geometries within the framework of the generalized Sobolev theory (i.e. non-local contributions to the radiation field are taken into account). As a first application, the role of rotation on YY Orionis line profiles is considered, using a kinematic model which combines rotation and collapse. One result of this investigation is that the line profiles calculated for the angular momentum values which are in rough agreement with the value expected from the differential galactic rotation do not qualitatively differ from profiles computed assuming radial collapse.
No associations
LandOfFree
Spectral line formation in axisymmetric moving envelopes - Method and application to YY Orionis stars 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 Spectral line formation in axisymmetric moving envelopes - Method and application to YY Orionis stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral line formation in axisymmetric moving envelopes - Method and application to YY Orionis stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1442035