New optical nova candidate in M 31

Details New optical nova candidate in M 31 New optical nova candidate in M 31

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2383....1b&link_type=abstract

The Astronomer's Telegram, #2383

Astronomy and Astrophysics

Astronomy

Optical, Cataclysmic Variables, Novae, Transients

Scientific paper

We report the discovery of a possible nova in M 31 on two 10x60s stacked R filter CCD images obtained with the robotic 60cm telescope with an E2V CCD (2kx2k, 13.5 micron sq. pixels) of the Livermore Optical Transient Imaging System (Super-LOTIS, located at Steward Observatory, Kitt Peak, Arizona, USA) on 2010 January 11.13 and 12.09 UT with respective R magnitudes of 17.6, 16.3.

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