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Recurrent Novae in M31
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SYSNO ASEP 0444954 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Recurrent Novae in M31 Author(s) Shafter, A.W. (US)
Henze, M. (DE)
Rector, T. A. (US)
Schweizer, F. (US)
Hornoch, Kamil (ASU-R) ORCID
Orio, M. (IT)
Pietsch, W. (DE)
Darnley, M.J. (GB)
Williams, S.C. (GB)
Bode, M.F. (GB)
Bryan, J. (US)Source Title Astrophysical Journal Supplement Series. - : IoP Publishing - ISSN 0067-0049
Roč. 216, č. 2 (2015), 34/1-34/35Number of pages 35 s. Publication form Print - P Language eng - English Country US - United States Keywords individual (M31) galaxies ; stellar content ; cataclysmic variables Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics Institutional support ASU-R - RVO:67985815 UT WOS 000350899000013 DOI 10.1088/0067-0049/216/2/34 Annotation he reported positions of 964 suspected nova eruptions in M31 recorded through the end of calendar year 2013 have been compared in order to identify recurrent nova (RN) candidates. To pass the initial screen and qualify as a RN candidate, two or more eruptions were required to be coincident within 0'.1, although this criterion was relaxed to 0'.15 for novae discovered on early photographic patrols. A total of 118 eruptions from 51 potential RN systems satisfied the screening criterion. To determine what fraction of these novae are indeed recurrent, the original plates and published images of the relevant eruptions have been carefully compared. This procedure has resulted in the elimination of 27 of the 51 progenitor candidates (61 eruptions) from further consideration as RNe, with another 8 systems (17 eruptions) deemed unlikely to be recurrent. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2016
Number of the records: 1