Optical spectroscopy of novae in M 31

Details Optical spectroscopy of novae in M 31 Optical spectroscopy of novae in M 31

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010an....331..197d&link_type=abstract

Astronomische Nachrichten, Vol.331, Issue 2, p.197

Astronomy and Astrophysics

Astronomy

2

Galaxies: Individual (M 31), Novae, Cataclysmic Variables

Scientific paper

We report results of a spectrophotometric survey of novae in M 31. The observations were carried out using the TNG at La Palma and the 1.82 m telescope of the INAF/OAPD at Asiago observatory . Low resolution spectra of the novae, obtained mainly in the early decline phase, allow us to classify the objects following the Tololo scheme \citep{1992AJ....104..725W}
Based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundacin Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias, and based on observations collected at Asiago observatory.

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