Published in

Cambridge University Press, Proceedings of the International Astronomical Union, S285(7), p. 301-302, 2011

DOI: 10.1017/s1743921312000865

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Characterising the Dwarf Nova Population of the Catalina Real-time Transient Survey

Journal article published in 2011 by Deanne de Budè, Patrick Woudt ORCID, Brian Warner
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Data provided by SHERPA/RoMEO

Abstract

AbstractResults of a high-speed photometric study of dwarf novæ in the Catalina Real-time Transient Survey are given. A population of faint dwarf novæ near the orbital period minimum is detected. At the shortest periods there is a correlation between orbital period and outburst interval.