Spectroscopic confirmation of an optical nova in M31

Details Spectroscopic confirmation of an optical nova in M31 Spectroscopic confirmation of an optical nova in M31

Feb 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1009....1p&link_type=abstract

The Astronomer's Telegram, #1009

Astronomy and Astrophysics

Astronomy

2

Optical, Novae

Scientific paper

We report the spectroscopic confirmation of an optical nova candidate in M31 (RA=00:41:40.32, Dec=+41:14:33.5, J2000) discovered by K. Hornoch on 2007 Feb. 3.798 UT. The spectrum was taken using the Russian 6 m telescope and SCORPIO spectral camera on 2007 Feb. 13.674 UT. The spectrum covers the range 340-760 nm, resolution 1.3 nm. The spectrum shows strong Balmer emission lines (H_alpha FWHM=1760 km/s), FeII emission lines, and possibly weak He and N lines.

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