Mass Loss Rates in Central Stars of Planetary Nebulae-Reference-Cited by-同舟云学术

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Mass Loss Rates in Central Stars of Planetary Nebulae

Published:1989 Issue: Volume: Page:293-300
ISSN:
Container-title:Planetary Nebulae
language:
Short-container-title:

Author:

Perinotto M.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-009-0865-9_105.pdf

Reference37 articles.

1. Abbott, D.C. and Lucy, L.B. 1985, Ap.J. 288, 679

2. Adam, J. and Koppen, S. 1985, Astron. Astrophys. 142, 461 (AK)

3. Adams, S., Seaton, M.J., Howarth, I.D., Aurière, M. and Walsh, J.R. 1984, M.N.R.A.S. 207, 471 (ASHAW)

4. Bianchi, L., Cerrato, S. and Grewing, M. 1986, Astron. Astrophys. 169, 227 (BCG)

5. Bombeck, G., Koppen, J. and Bastian, U. 1986, in ESA SP-263, p. 287 (BKB)

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1. The dense and asymmetric central star wind of the young PN He 2−138;Monthly Notices of the Royal Astronomical Society;2009-12-11

2. H- and He-burning Central Stars and the Evolution to White Dwarfs;Symposium - International Astronomical Union;2003

3. Evolutionary Tracks;Symposium - International Astronomical Union;1993

4. Evolutionary Tracks;Planetary Nebulae;1993

5. Transformation of AGB stars into white dwarfs;White Dwarfs

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