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Line profiles in expanding envelopes

Authors: Surdej, Jean;

Line profiles in expanding envelopes

Abstract

An attempt is made to show how the physical and geometrical parameters prevailing in an expanding stellar envelope can be inferred from an analysis of one or more observed line profiles. Attention is given to the Sobolev approximation, line formation in outwardly accelerating envelopes, effects of a stellar core, and radiative transfer in outwardly decelerating envelopes. General equations are derived for both types of envelope, and some typical solutions are presented. Application of the method to P Cygni lines is discussed.

Country
Belgium
Related Organizations
Keywords

Aérospatiale, astronomie & astrophysique, Physique, chimie, mathématiques & sciences de la terre, RADIATIVE TRANSFER, STELLAR ENVELOPES, STELLAR MODELS, QUASARS, Physical, chemical, mathematical & earth Sciences, STELLAR EVOLUTION, EMISSION SPECTRA, Space science, astronomy & astrophysics, LINE SHAPE, STELLAR STRUCTURE

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green