On the generation of mass loss in cool giant stars due to propagating shock waves

Author:

Cuntz Manfred

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 30 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. The Wind Temperature and Mass-loss Rate of Arcturus (K1.5 III);The Astrophysical Journal;2022-06-01

2. Atmospheric Heating and Wind Acceleration in Cool Evolved Stars;Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems;2014-11-25

3. Basal chromospheric flux and Maunder Minimum-type stars: the quiet-Sun chromosphere as a universal phenomenon;Astronomy & Astrophysics;2012-04

4. Chromosphere of K giant stars;Astronomy & Astrophysics;2011-11

5. TESTING A PREDICTIVE THEORETICAL MODEL FOR THE MASS LOSS RATES OF COOL STARS;The Astrophysical Journal;2011-10-14

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