Spectroscopy of M31N 1995-11e: Not a Nova, but a Luminous Mira Variable in M31

Details Spectroscopy of M31N 1995-11e: Not a Nova, but a Luminous Mira Variable in M31 Spectroscopy of M31N 1995-11e: Not a Nova, but a Luminous Mira Variable in M31

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1834....1s&link_type=abstract

The Astronomer's Telegram, #1834

Astronomy and Astrophysics

Astronomy

4

Optical, Novae, Transients

Scientific paper

Recent photometric monitoring of M31 by two of us (K. Nishiyama and F. Kabashima) has revealed that the M31 nova candidate M31N 1995-11e (Nova 1995-08 in Shafter & Irby 2001, ApJ, 563, 749) has re-brightened over the past several months. The object was detected again on 2008 July 6.8 UT at m ~ 18.6 (unfiltered), and has remained detectable up to the present, reaching a peak brightness of m ~ 18 on 2008 September 9 UT.

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