Detailed analysis of cool stars-Reference-Cited by-同舟云学术

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Detailed analysis of cool stars

Published:1988-06 Issue:1 Volume:145 Page:61-115
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Proust D.,Foy R.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00645695.pdf

Reference68 articles.

1. Arp, H. C.: 1961, ?Stellar Content of Galaxies?,IAU Symp. 15.

2. Barbuy, B.: 1978,Astron. Astrophys. 67, 339.

3. Bell, R. A., Eriksson, K., Gustafsson, B., and Nördlund, A.: 1976,Astron. Astrophys. Suppl. Ser. 23, 37.

4. Blackwell, D. E., Ibbeston, P. A., and Willis, A. D.: 1976,Monthly Notices Roy. Astron. Soc. 177, 227.

5. Boyle, R. and McClure, R. D.: 1975,Publ. Astron. Soc. Pacific 87, 17.

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1. Fundamental properties of red-clump stars from long-baseline H-band interferometry;Astronomy & Astrophysics;2018-08

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3. THE VELOCITY DISTRIBUTION OF NEARBY STARS FROMHIPPARCOSDATA. I. THE SIGNIFICANCE OF THE MOVING GROUPS;The Astrophysical Journal;2009-07-16

4. A study of Kapteyn's star;Astronomy & Astrophysics;2005-07-18

5. A Survey of Proper Motion Stars. XIII. The Halo Population;The Astronomical Journal;1996-08

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