Spectroscopic confirmation of M31 nova candidate, M31N 2011-06d

Details Spectroscopic confirmation of M31 nova candidate, M31N 2011-06d Spectroscopic confirmation of M31 nova candidate, M31N 2011-06d

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3533....1c&link_type=abstract

The Astronomer's Telegram, #3533

Astronomy and Astrophysics

Astronomy

Optical, Ultra-Violet, X-Ray, Cataclysmic Variable, Nova

Scientific paper

A spectrum of the recent nova candidate M31N 2011-06d (= PNV J00430685+4115308 on CBAT/TOCP; H-alpha reported in ATEL#3486, ATEL# 3499) was obtained on July 26 with the Double Spectrograph mounted on the Palomar 200-inch Hale telescope. The phase of the transient was about 18 days after its maximum light. The spectrum exhibits prominent Balmer emission lines (FWHM Halpha ~ 1,700 km/s), OI 8446 and 7773 lines as well as Fe II emission lines.

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