Article (Scientific journals)
Formation of P Cygni Line Profiles in Relativistically Expanding Atmospheres. II. The Effect of the Continuum Frequency Shape and Limb Darkening of the Core
Hutsemekers, Damien
1993In Astrophysical Journal, 417, p. 97-101
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The authors thank SAO/NASA ADS Astronomy Abstract Service and American Astronomical Society for their deposit authorization. The original publication can be found in the Astrophysical Journal.


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Keywords :
LINE: FORMATION; LINE: PROFILES; GALAXIES: QUASARS: GENERAL; RADIATIVE TRANSFER; RELATIVITY
Abstract :
[en] Abstract image available at: http://adsabs.harvard.edu/abs/1993ApJ...417...97H
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Hutsemekers, Damien ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astroph. extragalactique et observations spatiales (AEOS)
Language :
English
Title :
Formation of P Cygni Line Profiles in Relativistically Expanding Atmospheres. II. The Effect of the Continuum Frequency Shape and Limb Darkening of the Core
Publication date :
01 November 1993
Journal title :
Astrophysical Journal
ISSN :
0004-637X
eISSN :
1538-4357
Publisher :
University of Chicago Press, Chicago, United States - Illinois
Volume :
417
Pages :
97-101
Peer reviewed :
Peer Reviewed verified by ORBi
Available on ORBi :
since 10 March 2010

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