From Miras to Planetary Nebulae: A Model of Mass Loss-Reference-Cited by-同舟云学术

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From Miras to Planetary Nebulae: A Model of Mass Loss

Published:1986 Issue: Volume: Page:119-126
ISSN:0067-0057
Container-title:Light on Dark Matter
language:
Short-container-title:

Author:

Bedijn P. J.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-009-4672-9_27.pdf

Reference18 articles.

1. Baud, B, Habing, H.J.: 1983, Astron. Astrophys. 127, 73

2. Bedijn, P.J.: 1985, Astron. Astrophys., submitted

3. Feast, M.W. 1984, Monthly Notices Roy. Astron. Soc. 211, 51 P

4. Feast, M.W. 1984, Monthly Notices Roy. Astron. Soc. 211, in press

5. Fox, M.W., Wood, P.R.: 1982, Astrophys. J. 259, 198

Cited by 13 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 Impact of Space Experiments on Our Knowledge of the Physics of the Universe;The Impact of Space Experiments on Our Knowledge of the Physics of the Universe;2004

2. Mass loss mechanisms in evolved stars;The Astronomy and Astrophysics Review;1991

3. The Effect of Dust Shell Emission on the Strengths of Infrared Spectral Features in OH/IR Stars;Publications of the Astronomical Society of Australia;1990

4. Winds of Late Type Stars;Reviews in Modern Astronomy;1990

5. OH/IR Stars and other IRAS Point Sources as Progenitors of Planetary Nebulae;Symposium - International Astronomical Union;1989

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