Abstract
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 (Williams 1992). © 2010 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim.
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APA
Di Mille, F., Orio, M., Ciroi, S., Bianchini, A., Rafanelli, P., & Nelson, T. (2010). Optical spectroscopy of novae in M 31. Astronomische Nachrichten, 331(2), 197–200. https://doi.org/10.1002/asna.200911326
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