M31N2008-11b is a Galactic Dwarf Nova

Details M31N2008-11b is a Galactic Dwarf Nova M31N2008-11b is a Galactic Dwarf Nova

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1867....1k&link_type=abstract

The Astronomer's Telegram, #1867

Astronomy and Astrophysics

Astronomy

2

Cataclysmic Variables, Novae, Transients, Variables

Scientific paper

We observed M31N2008-11b >(K. Itagaki, CBET#1588) with the Double Beam Spectrograph on the Palomar Hale 5-m telescope on UT Dec 4.221. This spectrum has a steep blue continuum, very narrow emission in H-alpha and broad absorption in H-beta through at least H-eta. Further, there is a faint blue counterpart in SDSS DR Supplement g-band imaging (g=22.8, r > 23.3).

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