M31N 2010-10b: A Slowly-Evolving, Fe II Nova in M31

Details M31N 2010-10b: A Slowly-Evolving, Fe II Nova in M31 M31N 2010-10b: A Slowly-Evolving, Fe II Nova in M31

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.3039....1s&link_type=abstract

The Astronomer's Telegram, #3039

Astronomy and Astrophysics

Astronomy

1

Optical, Nova, Transient

Scientific paper

We report spectroscopic observations of the M31 nova candidate M31N 2010-10b, which was discovered by one of us (KH) on 2010 Aug. 19.055 UT (CBET #2487). At our request, a series of spectra (410-900 nm) of M31N 2010-10b were obtained on 2010 Oct. 28.31, Nov. 03.31, and Nov. 11.28 UT with the 9.2m Hobby-Eberly Telescope (+ Marcario Low-Resolution Spectrograph). The early spectra were characterized by narrow (unresolved) Balmer (FWHM Hα < 600 km/s) and Ca II infrared triplet emission features superimposed on a blue continuum.

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