Location via proxy:   [ UP ]  
[Report a bug]   [Manage cookies]                

A publishing partnership

Multiple Outbursts of a Cataclysmic Variable in the Globular Cluster M22

, , , , , , , , , , , , , , , , , , , , , and

Published 2005 January 24 © 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation I. A. Bond et al 2005 ApJ 620 L103 DOI 10.1086/428836

1538-4357/620/2/L103

Abstract

We present a 4 yr light curve of a cataclysmic variable in M22, based on an analysis of accumulated data from the Microlensing Observations in Astrophysics (MOA) microlensing survey. The position of the star coincides with that of a transient event observed by the Hubble Space Telescope (HST) in 1999, originally attributed to microlensing but later suspected to be a dwarf nova outburst. Two outburst episodes, one in 2002 and one in 2003, with ΔI ~ 3 are seen in the MOA data, thus confirming that the HST event was a dwarf nova outburst. The MOA and HST data show that this dwarf nova underwent at least three outburst episodes during 1999-2004. Further close monitoring of this event is encouraged, as future outburst episodes are expected.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/428836