Optical spectroscopy of novae in M 31

F. Di Mille; M. Orio; S. Ciroi; A. Bianchini; P. Rafanelli; T. Nelson

doi:10.1002/asna.200911326

Optical spectroscopy of novae in M 31

F. Di Mille
, M. Orio
, S. Ciroi
, A. Bianchini
, P. Rafanelli
, T. Nelson

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

5 Scopus citations

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).

Original language	English (US)
Pages (from-to)	197-200
Number of pages	4
Journal	Astronomische Nachrichten
Volume	331
Issue number	2
DOIs	https://doi.org/10.1002/asna.200911326
State	Published - Feb 2010

Keywords

Cataclysmic variables
Galaxies: Individual (M 31)
Novae

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10.1002/asna.200911326

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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).",

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T1 - Optical spectroscopy of novae in M 31

AU - Di Mille, F.

AU - Orio, M.

AU - Ciroi, S.

AU - Bianchini, A.

AU - Rafanelli, P.

AU - Nelson, T.

PY - 2010/2

Y1 - 2010/2

N2 - 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).

AB - 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).

KW - Cataclysmic variables

KW - Galaxies: Individual (M 31)

KW - Novae

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UR - https://www.scopus.com/pages/publications/77952512219#tab=citedBy

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DO - 10.1002/asna.200911326

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JO - Astronomische Nachrichten

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ER -

Optical spectroscopy of novae in M 31

Abstract

Keywords

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