Spectroscopic classification of the M31 nova candidate, M31N 2011-06a

Details Spectroscopic classification of the M31 nova candidate, M31N 2011-06a Spectroscopic classification of the M31 nova candidate, M31N 2011-06a

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3497....1c&link_type=abstract

The Astronomer's Telegram, #3497

Astronomy and Astrophysics

Astronomy

Optical, Nova

Scientific paper

A spectrum of the nova candidate M31N 2011-06a (ATEL#3409) was obtained with the Double Beam Spectrograph mounted on the Palomar 200-inch Hale telescope on June 28, 2011, about 20 days after its maximum light. The spectrum exhibits prominent Balmer emission lines (FWHM Halpha ~ 2000 km/s) and Fe II emission lines. This observation confirms that M31N 2011-06a is a classical nova, and a member of the Fe II spectroscopic class (Williams et al.

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