Generalized energy balance method for the determination of central star parameters and optical thickness of a planetary nebula-Reference-Cited by-同舟云学术

Generalized energy balance method for the determination of central star parameters and optical thickness of a planetary nebula

Published:1995 Issue:1 Volume:232 Page:99-129
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Malkov Yu. F.,Golovatyj V. V.,Rokach O. V.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00627547.pdf

Reference71 articles.

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3. Adams, S. and Seaton, M.: 1982,Monthly Notices Roy. Astron. Soc. 200, 7p.

4. Adams, S., Seaton, M.J., Howarth, I.D., Auri�re, M., and Walsh, J.R.: 1984,Monthly Notices Roy. Astron. Soc. 207, 471.

5. Aldrovandi, S.M.V. and Pequignot, D.: 1973,Astron. Astrophys. 25, 137.

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