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Improved modelling for spatially resolved spectroscopy of a P Cyg envelope

Published online by Cambridge University Press:  26 May 2016

M. Bourguine  and
A. Chalabaev
M. Bourguine
Affiliation:
CNRS, Observatoire de Grenoble, UJF-B.P.53X,38041 Grenoble CEDEX France FIAN Astro-space Center, Moscow, Russia
A. Chalabaev
Affiliation:
CNRS, Observatoire de Grenoble, UJF-B.P.53X,38041 Grenoble CEDEX France

Extract

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Our study, of which we give here a progress report, addresses two problems. The first is to develop methods and software permitting to compare a wide range of theoretical models of stars with envelopes with observational data produced or expected to be produced by high angular resolution optical interferometry combined with spectroscopy. The second problem is to find out the modes of interferometric observations (base length, spectral resolution etc) that are most informative for determining the physical parameters of stellar envelopes.

Type
7. OB Stellar Winds
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 502 - 504
Copyright
Copyright © Kluwer 1994 

References

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