The UV spectrum of the Be star 88 Herculis-Reference-Cited by-同舟云学术

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The UV spectrum of the Be star 88 Herculis

Published:1990 Issue:1 Volume:174 Page:49-90
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Danezis E.,Theodossiou E.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00645654.pdf

Reference22 articles.

1. Barylak, M. and Doazan, V.: 1986,Astron. Astrophys. 159, 65.

2. Bauer Hagen, W. and Stencel, R.: 1989,Astrophys. J. 69, 667.

3. Bidelman, W. P. and Svolopoulos, S. N.: 1960,Publ. Astron. Soc. Pacific 72, 129.

4. Danezis, E. and Theodossiou, E.: 1988,Astron. Astrophys. Suppl. Ser. 72, 497.

5. Doazan, V.: 1973,Astron. Astrophys. 27, 395.

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1. The Cu II Spectrum;Atoms;2017-02-24

2. Experimental stark widths of six UV lines of ZnII;Journal of Physics B: Atomic, Molecular and Optical Physics;2008-11-10

3. Experimental oscillator strengths of Zn II lines of astrophysical interest;The European Physical Journal D;2005-10-25

4. Ultraviolet Spectrophotometry of Variable Early‐Type Be and B Stars Derived from High‐ResolutionIUEData;The Astrophysical Journal;2001-12

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