Swift UVOT detection of PNV J00422413+4111549: a very fast nova in M 31 or a flaring foreground star?

Details Swift UVOT detection of PNV J00422413+4111549: a very fast nova in M 31 or a flaring foreground star? Swift UVOT detection of PNV J00422413+4111549: a very fast nova in M 31 or a flaring foreground star?

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3446....1p&link_type=abstract

The Astronomer's Telegram, #3446

Astronomy and Astrophysics

Astronomy

Optical, Ultra-Violet, X-Ray, Nova, Star

Scientific paper

The optical light curve of the nova candidate PNV J00422413+4111549
(candidate three in ATel #3409) can be constrained using two deep M 31
observations obtained with the 0.65-m telescope at Ondrejov (K. Hornoch)
where the source is not detected 1.4 days before and 5.6 days after the
discovery (see Table).

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