2003A&A...399..695K


Query : 2003A&A...399..695K

2003A&A...399..695K - Astronomy and Astrophysics, volume 399695-697 (2003/2-4)

CK Vul as a candidate eruptive stellar merging event.

KATO T.

Abstract (from CDS):

CK Vul (Nova Vul 1670) is one of the most mysterious objects among erupting stellar objects. Past studies have suggested that CK Vul is a final helium-flash object resembling V605 Aql and V4334 Sgr (Sakurai's object). The peculiar outburst light curve of CK Vul, however, had no similar counterpart among the known eruptive objects. Furthermore, the presence of hydrogen in the proposed remnant seems to contradict with the final helium-flash scenario. We propose that the peculiarities of CK Vul can be naturally understood if we consider a merging of main-sequence stars, following a new interpretation by Soker & Tylenda (2003ApJ...582L.105S) which was proposed to explain the peculiar eruptive object V838 Mon. In this case, the 1670 outburst of CK Vul may be best understood as a V838 Mon-like event which occurred in our vicinity.

Abstract Copyright: ∼

Journal keyword(s): accretion, accretion disks - stars - novae, cataclysmic variables - stars: individual: CK Vul

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* V838 Mon CV* 07 04 04.8221494992 -03 50 50.648894412       15.181 14.51 M10+B3V 462 1
2 V* V4334 Sgr CV* 17 52 32.69352 -17 41 08.0160           F2Ia 390 0
3 PN A66 58 PN 19 18 20.476 +01 46 59.62           [WC4] 327 0
4 V* CK Vul CV* 19 47 37.9577343864 +27 18 41.792401368           ~ 159 0

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