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X-ray line profiles from structured stellar winds

Published online by Cambridge University Press:  26 May 2016

Lidia M. Oskinova ,
Achim Feldmeier  and
Wolf-Rainer Hamann
Lidia M. Oskinova
Affiliation:
Lehrstuhl Astrophysik, Institut für Physik, Universität Potsdam, Am Neuen Palais 10, D-14469 Potsdam, BRD
Achim Feldmeier
Affiliation:
Lehrstuhl Astrophysik, Institut für Physik, Universität Potsdam, Am Neuen Palais 10, D-14469 Potsdam, BRD
Wolf-Rainer Hamann
Affiliation:
Lehrstuhl Astrophysik, Institut für Physik, Universität Potsdam, Am Neuen Palais 10, D-14469 Potsdam, BRD

Abstract

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Absorbing material compressed in a number of thin shells is effectively less opaque for X-rays than smoothly distributed gas. The calculated X-ray emission-line profiles are red-shifted if the emission arises from the starward side of the shells.

Type
Part 1. Atmospheres of Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 214 - 215
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Cassinelli, J.P., Miller, N.A., Waldron, W.L., et al. 2001, ApJ 554, 55.Google Scholar
Feldmeier, A., Puls, J., Pauldrach, A.W.A. 1997, A&A 322, 878.Google Scholar
Puls, C.A., Kudritzki, R.-P., Herrero, A., et al. 1996, A&A 305, 171.Google Scholar