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Mass Accretion in Intermediate Polar V1223 Sgr

Published online by Cambridge University Press:  21 February 2013

Ladislav Hric ,
Emil Kundra  and
Rudolf Gális
Ladislav Hric
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia email: hric@ta3.sk
Emil Kundra
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia email: hric@ta3.sk
Rudolf Gális
Affiliation:
Department of Theoretical Physics and Astrophysics, Institute of Physics, Faculty of Sciences, P. J. Šafárik University, Park Angelinum 9, 040 01 Košice, Slovakia
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Abstract

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Intermediate polars (IPs) represent more than 70% of all cataclysmic variables (CVs) detected by INTEGRAL in hard X-ray. Nevertheless, only a quarter of all known IPs have been detected in this spectral band. This fact can be related to the activity state of these object ruled by changes in the mass accretion rate.

Keywords

Stars: novaecataclysmic variablesaccretionaccretion disks
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 225 - 226
Copyright
Copyright © International Astronomical Union 2013

References

Gális, R., Eckert, D., Paltani, S., Münz, F., & Kocka, M. 2009, Baltic Astronomy, 18, 321Google Scholar
Patterson, J. 1994, Publ. Astron. Soc. Pacific 106, 209CrossRefGoogle Scholar