Flare stars: Postflare behaviour of emission lines-Reference-Cited by-同舟云学术

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Flare stars: Postflare behaviour of emission lines

Published:1984 Issue:1 Volume:106 Page:1-34
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Gurzadyan G. A.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00653910.pdf

Reference16 articles.

1. Brown, R. T.: 1971,Astrophys. J. 170, 387.

2. Butler, C. J., Byrne, P. B., Andrews, A. D., and Doyle, J. G.: 1981,Monthly Notices Roy. Astron. Soc. 197, 815.

3. Gerschberg, R. E. and Chugainov, P. F.: 1967,Astron. J. USSR 44, 260.

4. Gurzadyan, G. A.: 1967,Doklady Acad. Nauk SSSR 172, 287.

5. Gurzadyan, G. A.: 1969,Planetary Nebulae, Gordon and Breach, New York.

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3. Dynamics of flares on late type dMe stars;Astronomy & Astrophysics;2003-01

4. On negative infrared flares of flare stars;The Astrophysical Journal;1988-09

5. Coordinated Photometry, Spectroscopy and X-ray Observations of Flare Stars;Activity in Cool Star Envelopes;1988

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