Spectroscopic Observations of Two Recent M31 Novae: M31N 2010-09b and M31N 2010-10a

Details Spectroscopic Observations of Two Recent M31 Novae: M31N 2010-09b and M31N 2010-10a Spectroscopic Observations of Two Recent M31 Novae: M31N 2010-09b and M31N 2010-10a

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2909....1s&link_type=abstract

The Astronomer's Telegram, #2909

Astronomy and Astrophysics

Astronomy

Optical, Nova, Transient

Scientific paper

We report spectroscopic observations of the recent M31 nova M31N 2010-09b (CBET #2472; ATel #2896), and of a new M31 nova candidate, M31N 2010-10a, which was discovered by Nishiyama and Kabashima (Miyaki- Argenteus Observatory, Japan) on 2010 Oct. 05.551 UT (private communication).
A previous spectrum of M31N 2010-09b obtained by our group within a day of discovery (Shafter et al., ATel #2898) established that the nova was likely a member of the Fe II class, but the possibility that it might evolve into a hybrid nova could not be ruled out at that time.

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