The system AM Her = 4U 1814 + 50
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/article/10.1007/BF00168043/fulltext.html
Reference106 articles.
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4. Bailey, J. A. et al.: 1978, Monthly Notices Roy. Astron. Soc. 184, 73P.
5. Berg, A. R. and Duthie, J. G.: 1977, Astrophys. J. 211, 859.
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1. Possible detection of TeV gamma rays from AM Herculis;The Astrophysical Journal;1991-03
2. Corrugation instability of a strong parallel slow shock wave. I. Numerical calculations for the case of a radiative shock;Astrophysics;1990
3. Spectral models of AM Her stars;Astrophysics and Space Science;1987-03
4. ?Swinging dipoles? inmagnetic close binary stars;Astrophysics and Space Science;1987-03
5. Spectral Models of AM Her Stars;International Astronomical Union Colloquium;1987
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