Similarities and differences in the spectral behavior of W Ser and UX Mon in the ultraviolet-Reference-Cited by-同舟云学术

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Similarities and differences in the spectral behavior of W Ser and UX Mon in the ultraviolet

Published:2013-01-03 Issue:2 Volume:344 Page:405-416
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Sanad M. R.,Bobrowsky M.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s10509-012-1343-8.pdf

Reference38 articles.

1. Andersen, J., Nordstrom, B.: Space Sci. Rev. 50, 179A (1989)

2. Bauer, C.: Astrophys. J. 101, 208B (1945)

3. Bruhweiler, F.: Private communication (2002)

4. Etzel, P.B., van den Bergh, H.: Astron. Astrophys. Suppl. Ser. 192, 1208E (1998)

5. Gaposchkin, S.: Astrophys. J. 105, 258G (1947)

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1. Ultraviolet spectroscopy of V Sagittae in high, intermediate and low states from HST and IUE satellites;Astrophysics and Space Science;2015-10-29

2. Non-conservative mass transfers in Algols;Monthly Notices of the Royal Astronomical Society;2014-05-03

3. ULTRAVIOLET SPECTROSCOPIC ANALYSIS OF TRANSIENT MASS FLOW OUTBURST IN U CEPHEI;The Astrophysical Journal;2013-09-03

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