Spectroscopic confirmation of recent M31 novae

Details Spectroscopic confirmation of recent M31 novae Spectroscopic confirmation of recent M31 novae

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3649....1c&link_type=abstract

The Astronomer's Telegram, #3649

Astronomy and Astrophysics

Astronomy

Optical, Cataclysmic Variable, Nova, Transient

Scientific paper

We report spectroscopic confirmation of M31N 2011-07a, M31N 2011-07b, M31N 2011-08a, M31N 2011-08b. The spectra were acquired with the Double Spectrograph mounted on the 200-inch Hale telescope at Palomar Observatory.
The spectrum of M31N 2011-07a (internally designated as PTF11kie) was obtained on Sept 03.461. The spectrum has a weak continuum and prominent line emissions --- Balmer series, C II 4267, Ne III 4640, He II 4686, Ne I 5686, N II 5679, C II 7234, O I 8446 and N I 9396.

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