The 'Alternative X' question - What causes the strong molecular bands and damping lines in very strong lined (super-metal-rich) stars?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by 16 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 Last Measurements Made with the Wampler Scanner. IV. Semicontinuous Scans of G and K Stars;Publications of the Astronomical Society of the Pacific;2009-08
2. The Benchmark Cluster Reddening Project. III. A Comparison of Reddening Values Derived from F and K Stars in NGC 752;The Astronomical Journal;2007-07-09
3. A rigorous statistical test for the existence of supermetallicity in F, G and K dwarfs;Monthly Notices of the Royal Astronomical Society;2006-06-01
4. A statistical search for supermetallicity in F, G and K stars;Monthly Notices of the Royal Astronomical Society;2002-02
5. The Upper end of the Galactic Metallicity Scale;New Quests in Stellar Astrophysics: The Link Between Stars and Cosmology;2002
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