Constraining the time of outburst of an optical nova candidate in M 31

Details Constraining the time of outburst of an optical nova candidate in M 31 Constraining the time of outburst of an optical nova candidate in M 31

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2189....1h&link_type=abstract

The Astronomer's Telegram, #2189

Astronomy and Astrophysics

Astronomy

2

Optical, Novae

Scientific paper

We confirm a nova candidate in M 31 reported to us by K. Nishiyama and F. Kabashima and present a pre-discovery detection that allows us to tightly constrain the time of outburst for this object. The nova candidate was discovered by Nishiyama and Kabashima (Miyaki-Argenteus observatory, Japan) on 2009 September 3.752 UT, with no object visible at its position on September 1.566 UT (private communication).

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