Počet záznamů: 1
Recurrent Novae in M31
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SYSNO ASEP 0444954 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Recurrent Novae in M31 Tvůrce(i) 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)Zdroj.dok. Astrophysical Journal Supplement Series. - : IoP Publishing - ISSN 0067-0049
Roč. 216, č. 2 (2015), 34/1-34/35Poč.str. 35 s. Forma vydání Tištěná - P Jazyk dok. eng - angličtina Země vyd. US - Spojené státy americké Klíč. slova individual (M31) galaxies ; stellar content ; cataclysmic variables Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Institucionální podpora ASU-R - RVO:67985815 UT WOS 000350899000013 DOI 10.1088/0067-0049/216/2/34 Anotace 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. Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2016
Počet záznamů: 1