Spectroscopic Confirmation of the Nova Candidate M31N-2007-11c

Details Spectroscopic Confirmation of the Nova Candidate M31N-2007-11c Spectroscopic Confirmation of the Nova Candidate M31N-2007-11c

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1292....1c&link_type=abstract

The Astronomer's Telegram, #1292

Astronomy and Astrophysics

Astronomy

2

Optical, Novae

Scientific paper

We confirm spectroscopically the optical nova candidate M31N-2007-11c reported in ATEL #1275 (see also CBAT M31 nova page). A 2700 sec spectrum (range 360-750 nm; 2.7-nm resolution) was obtained on 2007 Nov 16.95 with the Asiago 1.82 m telescope (+ AFOSC). The spectrum shows a blue continuum and strong Balmer lines up to H-epsilon with H_alpha FWHM of about 1700 km/s.

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