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The Period Distribution of Supersoft Sources

Published online by Cambridge University Press:  12 April 2016

P. Kahabka*
Affiliation:
Astronomical Institute “Anton Pannekoek” and Center for High Energy Astrophysics, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands

Abstract

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The observed and predicted orbital period distributions of supersoft sources are in good agreement.

Type
Supernovae & Supersoft X-Ray Sources
Copyright
Copyright © Kluwer 1996

References

Kahabka, P., Trümper, J., 1995, in “IAU Symposium 165, Compact Stars in Binaries”, p 425 Google Scholar
Kahabka, P., 1995a, in “Cataclysmic Variables”, eds Bianchini, A. et al., Kluwer, p 435 Google Scholar
Kahabka, P., 1995b, A&A, 304, 227 Google Scholar
Rappaport, S., di Stephano, R., Smith, J.D., 1994, Ap. J., 270, L9 Google Scholar
van den Heuvel, E.P.J., Bhattacharya, D., Nomoto, K., et al., 1992, A&A, 262, 97 Google Scholar
Yungelson, L., Livio, M., Tutukov, A., Kenyon, S.J., 1996, Ap. J., submittedGoogle Scholar