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Magnetic CVs in the UCT CCD CV Survey

Published online by Cambridge University Press:  12 April 2016

Patrick A. Woudt  and
Brian Warner
Patrick A. Woudt
Affiliation:
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa
Brian Warner
Affiliation:
Department of Astronomy, University of Cape Town, Rondebosch 7700, South Africa

Abstract

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An overview is given of all the magnetic CVs found in the UCT CCD CV Survey (Woudt & Warner 2001, 2002, 2003a). We have identified eight new candidate Intermediate Polars (IP), of which six are classical novae (RR Cha, DD Cir, AP Cru, V697 Sco, V373 Sct, and RXJ1039.7-0507). The two other candidate IPs are Aqr1 (2236+0052) and RX J0944.5+0357. In addition, there are two probable Polars, namely V351 Pup (= Nova Puppis 1991) and FIRST J102347.6+003841.

Type
Part 1. Population and Evolution
Information
International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 39 - 45
Copyright
Copyright © Astronomical Society of the Pacific 2004

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