Spectral Classification and Estimation of Distances to the Be/X-Ray Binaries 1H1936+541 and 1H2202+501

Author:

Simon A. O.,Metlova N. V.,Godunova V. G.,Vasylenko V. V.

Publisher

Allerton Press

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference36 articles.

1. A Course in Astrophysics and Stellar Astronomy, Ed. by A. A. Mikhailov (Nauka, Moscow, 1951; Israel Program for Scientific Translations, Jerusalem, 1960), Vol. 1.

2. V. M. Lyutyi, “Automatic electrophotometer with photon counting,” Soobshch. GAISh, No. 172, 30–41 (1971).

3. K. M. Apparao, “X-ray emission from Be star/X-ray binaries,” Space Sci. Rev. 69, 255–329 (1994).

4. M. L. Arias, J. Zorec, L. Cidale, A. E. Ringuelet, et al., “Fe II emission lines in Be stars — I. Empirical diagnostic of physical conditions in the circumstellar discs,” Astron. Astrophys. 460, 821–829 (2006).

5. K. Belczynski and J. Ziolkowski, “On the apparent lack of Be X-ray binaries with black holes,” Astrophys. J. 707, 870–877 (2009).

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