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Properties of fast winds in hot stars in the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

P. Patriarchi  and
M. Perinotto
P. Patriarchi
Affiliation:
GNA/CNR c/o Osserv. Arcetri
M. Perinotto
Affiliation:
Dipartimento di Astronomia Univ. Firenze, L.go E. Fermi 5, I-50125 Firenze, Italy

Abstract

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We have studied with the SEI method (Sobolev approximation plus Exact Integration of the transfer equation) seven hot stars, five belonging to the Large Magellanic Cloud (LMC) and two to the Small Magellanic Cloud (SMC), which have been observed with IUE in high resolution. We present preliminary results of the work, i.e. the terminal velocities and the optical depth of the P Cygni profile. An evaluation of qiM has been done, as well as a comparison with previous work.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 360 - 362
Copyright
Copyright © Kluwer 1991 

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