Self-consistent and Time-dependent Magnetohydrodynamic Chromosphere Models for Magnetically Active Stars-Reference-Cited by-同舟云学术

Self-consistent and Time-dependent Magnetohydrodynamic Chromosphere Models for Magnetically Active Stars

Published:1998-02-01 Issue:2 Volume:493 Page:L117-L120
ISSN:0004-637X
Container-title:The Astrophysical Journal
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Author:

Cuntz Manfred,Ulmschneider Peter,Musielak Zdzislaw E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

1. Buchholz, B., Ulmschneider, P. & Cuntz, M. 1998, ApJ, in press

2. Chromospheric heating and metal deficiency in cool giants: Theoretical results versus observations

3. Hasan, S. S. & van Ballegooijen, A. A. 1997, in Cool Stars, Stellar Systems, and the Sun, 10th Cambridge Workshop: poster edition, ed. R. A. Donahue & J. A. Bookbinder (San Francisco: ASP), in press

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