Time Variability of the Ca II K Emission Line of Giants-Reference-Cited by-同舟云学术

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Time Variability of the Ca II K Emission Line of Giants

Published:2008-07 Issue:869 Volume:120 Page:730-739
ISSN:0004-6280
Container-title:Publications of the Astronomical Society of the Pacific
language:en
Short-container-title:PUBL ASTRON SOC PAC

Author:

Shetrone Matthew,Rivera Frances,Smith Graeme,Carveth Carol

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference25 articles.

1. Stellar model chromospheres. III - Arcturus /K2 III/

2. UBVRI photometry. II - The Cousins VRI system, its temperature and absolute flux calibration, and relevance for two-dimensional photometry

3. High-resolution stellar vidicon spectrophotometry. I - Variable mass loss from Arcturus and the hypothesis of giant convective elements

4. A. J. Deutsch, L. Houziaux, and H. E. Butler, 1970 , in IAY Symposium 36 , Ultraviolet Stellar Spectra and Related Groundbased Observations, ed. (Dordrecht: Dordrecht Reidel), p. 199

5. The formation of emission lines in the expanding chromospheres of luminous cool stars. I - The importance of atmospheric extension and partial redistribution effects

Cited by 1 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. Comparing the CaiiH and K Emission Lines in Red Giant Stars;Publications of the Astronomical Society of the Pacific;2009-08

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