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He I Line Profiles Obtained From a Be Wind Model

Published online by Cambridge University Press:  12 April 2016

R. Rohrmann
R. Rohrmann*
Affiliation:
Observatorio Astronómico, Laprida 854, 5000 Cordoba, Argentina

Abstract

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We undertook a non-LTE radiative transfer calculation to find out the possible conditions under which observed H and He I line profiles arise from some Be stars.

Type
6. Disks
Information
International Astronomical Union Colloquium , Volume 175: The Be Phenomenon in Early-Type Stars , 2000 , pp. 640 - 643
Copyright
Copyright © Astronomical Society of the Pacific 2000

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