Optical spectroscopy of novae in M 31

被引：5
作者：
Di Mille, F. [1 ,2 ]
Orio, M. [3 ,4 ]
Ciroi, S. [1 ]
Bianchini, A. [1 ]
Rafanelli, P. [1 ]
Nelson, T. [3 ,5 ]
机构：
[1] Univ Padua, Dipartimento Astron, I-35122 Padua, Italy
[2] Carnegie Inst Washington, Las Campanas Observ, La Serena, Chile
[3] INAF OAPD, I-35122 Padua, Italy
[4] Univ Wisconsin, Madison, WI 53706 USA
[5] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源：
ASTRONOMISCHE NACHRICHTEN | 2010年 / 331卷 / 02期
关键词：
galaxies: individual (M 31); novae; cataclysmic variables; SPECTRA; EVOLUTION; M31;
D O I：
10.1002/asna.200911326
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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) (C) 2010 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
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页码：197 / 200
页数：4
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