Spectroscopic confirmation of the nova close to the core of M 31 (ATel #2234) and brightness estimates of the novae M31N 2009-08a and M31N 2009-08e

Details Spectroscopic confirmation of the nova close to the core of M 31 (ATel #2234) and brightness estimates of the novae M31N 2009-08a and M31N 2009-08e Spectroscopic confirmation of the nova close to the core of M 31 (ATel #2234) and brightness estimates of the novae M31N 2009-08a and M31N 2009-08e

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2240....1f&link_type=abstract

The Astronomer's Telegram, #2240

Astronomy and Astrophysics

Astronomy

1

Optical, Cataclysmic Variables, Novae

Scientific paper

We obtained low resolution spectra of the optical nova candidate in M 31 (RA=00 42 45.76, Dec=+41 15 57.1, J2000) discovered by P. Podigachoski et al. (ATel #2234) on images, obtained on 2009 Oct 9.08 in H-alpha filter. The nova is very close (16" east and 12" south) to the core of M 31. The spectrum of the candidate has been taken on 2009 Oct. 9.820 UT with the Russian 6-m telescope (BTA) equipped with the SCORPIO spectral camera.

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