Discovery of a new outburst of the bipolar jet-emitter, stable H-burning WD in the symbiotic binary Hen 3-1341

Details Discovery of a new outburst of the bipolar jet-emitter, stable H-burning WD in the symbiotic binary Hen 3-1341 Discovery of a new outburst of the bipolar jet-emitter, stable H-burning WD in the symbiotic binary Hen 3-1341

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3946....1m&link_type=abstract

The Astronomer's Telegram, #3946

Astronomy and Astrophysics

Astronomy

Optical, Ultra-Violet, X-Ray, Cataclysmic Variable, Nova, Variables

Scientific paper

When a week ago we resumed the optical monitoring following its emergence from the conjunction with the Sun, we found that the symbiotic star Hen 3-1341 (V2523 Oph) is undergoing a bright outburst, the first one occurring since the last outburst that peaked in brightness in mid 1999. During the preceding quiescence, the object went down to B=14.179, V=13.353, Rc=12.053, Ic=10.861 on 2009 Sept 11.798 UT, and our last measurement before the current outburst reported it at B=13.948, V=13.231, Rc=11.798 and Ic=10.659 on 2011 July 3.909 UT.

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