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New Photometric Observations of RS Oph

Published online by Cambridge University Press:  17 January 2013

Irina Voloshina
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Universitetskij prospect 13, Moscow 119992, Russia email: vib@sai.msu.ru
Vladimir Metlov
Affiliation:
Sternberg Astronomical Institute, Moscow State University, Universitetskij prospect 13, Moscow 119992, Russia email: vib@sai.msu.ru
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Abstract

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The recurrent nova RS Oph is a long period (~455 days) binary system consisting of a hot white dwarf with mass close to the Chandrasekhar limit and an M-type giant secondary. Here we present the results of photometric observations of this nova which were made during recent years with the telescopes of the Sternberg Astronomical Institute in Crimea.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

References

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