Stellar model chromospheres. VII - Capella /G5 III +/, Pollux /K0 III/, and Aldebaran /K5 III/

Author:

Kelch W. L.,Chang S.-H.,Furenlid I.,Linsky J. L.,Basri G. S.,Chiu H.-Y.,Maran S. P.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 115 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. Resolving Red Giant Winds with the Hubble Space Telescope*;The Astrophysical Journal;2024-05-24

2. Stellar Model Chromospheres and Spectroscopic Diagnostics;Annual Review of Astronomy and Astrophysics;2017-08-18

3. Estimating the chromospheric magnetic field from a revised NLTE modelling: the case of HR 7428;Monthly Notices of the Royal Astronomical Society;2017-03-14

4. HUBBLE SPACE TELESCOPECONSTRAINTS ON THE WINDS AND ASTROSPHERES OF RED GIANT STARS;The Astrophysical Journal;2016-09-23

5. Chromospheric thermal continuum millimetre emission from non-dusty K and M red giants;Monthly Notices of the Royal Astronomical Society;2012-11-07

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