1996JAVSO..24...81G


Query : 1996JAVSO..24...81G

1996JAVSO..24...81G - J. Am. Assoc. Variable star obs., 24, 81-85 (1996/June-0)

The period of the symbiotic nova PU Vulpeculae.

GARNAVICH P.M.

Abstract (from CDS):

PU Vul is a very slowly evolving symbiotic nova. AAVSO observations spanning 15 years are used to show that the system is an eclipsing binary with a period of 13.42 + 0.02 years. Modeling of the eclipse shapes indicates that radii of both components of the binary have decreased between 1980 and 1994. The cause for the shrinkage in the size of the giant star is unknown.

Abstract Copyright: ∼

Journal keyword(s):

Simbad objects: 3

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Number of rows : 3
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* RT Ser Sy* 17 39 51.9832062720 -11 56 38.818883580   15.979 14.649 14.461   M7e 131 0
2 V* RR Tel Sy* 20 04 18.5404499712 -55 43 33.153979080 9.93 11.33 10.81 11.689   M5e 550 0
3 V* PU Vul Sy* 20 21 13.3111130136 +21 34 18.697391652   11.13 10.87 11.697   M3+F2Ib 319 0

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