Spectroscopic Confirmation and Classification of the Recent M33 Nova Candidate, M33N 2010-11a

Details Spectroscopic Confirmation and Classification of the Recent M33 Nova Candidate, M33N 2010-11a Spectroscopic Confirmation and Classification of the Recent M33 Nova Candidate, M33N 2010-11a

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.3063....1s&link_type=abstract

The Astronomer's Telegram, #3063

Astronomy and Astrophysics

Astronomy

1

Optical, Nova, Transient

Scientific paper

We report spectroscopic observations of the recent M33 nova candidate, M33N 2010-11a, which was discovered by Jiangao Ruan (Fangchenggang, Guangxi, China) and Xing Gao (Urumqi, Xinjiang, China) on 2010 Nov. 27.530 at m~18.6 (unfiltered), and independently by Koichi Nishiyama and Fujio Kabashima (Miyaki-Argenteus Observatory, Japan) approximately a day later on Nov. 28.542 UT. By the time of Nishiyama and Kabashima's observations the object had brightened to m~16.7 (unfiltered).

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