Confirmation and Spectroscopic Classification of the Recent M31 Nova Candidate, M31N 2010-10d

Details Confirmation and Spectroscopic Classification of the Recent M31 Nova Candidate, M31N 2010-10d Confirmation and Spectroscopic Classification of the Recent M31 Nova Candidate, M31N 2010-10d

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2987....1s&link_type=abstract

The Astronomer's Telegram, #2987

Astronomy and Astrophysics

Astronomy

1

Optical, Nova, Transient

Scientific paper

At our request a spectrum (410-910 nm) of the recent M31 nova candidate, M31N 2010-10d (CBET #2516), was obtained by John Caldwell on 2010 Oct. 30.31 UT (~1 day post discovery) with the Low-Resolution Spectrograph on the 9.2m Hobby-Eberly Telescope. The spectrum exhibits prominent Balmer and Fe II emission lines (FWHM Hα ~ 1100 km/s) flanked by weak P Cygni absorption features (Δ V ~ -1100 km/s) superimposed on a blue continuum.

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