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  VV Pup  
000-BBP-388 (4190 observations)  
Puppis Sequence
08 15 06.80 -19 03 18.0  (123.77833 -19.05500) Search nearby
B1950.0 08 12 52.24 -18 54 04.8
Galactic coord. 239.652 +8.713
Other names

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1RXS J081506.7-190310 2MASS J08150679-1903176 AAVSO 0810-18
Downes VV Pup    
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Variability type
Spectral type pec(cont+e)+M4-5V
Mag. range
13.9 - 18 V
Discoverer --
28 Mar 1935 (HJD 2427889.6474) Ephemeris
Outburst --
Period 0.0697468256 d  (100.4354289 min)
Rise/eclipse dur. --
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1 GCVS Team mu = 0.100", P = 165.0deg. The epoch of light maximum is given. The mean brightness varies by 2 - 3m. Intervals of active light variation with amplitude up to 2m during maximal mean brightness are observed. During low activity intervals when amplitude is about 0.3m mean brightness is minimal; during this time the ellipsoidal light variations of the system are observed in the range 15.1m - 15.3m J with the elements Min = 2427889.6509 + 0.0697468256d*E [D.A.Allen, A.M.Cherepashchuk, MN 201, 521, 1982.]. The white dwarf rotation period is equal to the orbital period. There are flickerings. Spectrum description [G.Williams, ApJ Suppl 53, N3, 523, 1983., J.Patterson, K.Beuermann, D.Q. Lamb, G.Fabbiano, J.C.Raymond, J.Swank, N.E.White, ApJ 279, 785, 1984.].
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1 Cyclotron Modeling Phase-Resolved Infrared Spectroscopy of Polars. II. EQ
Ceti, AN Ursa Majoris, and VV Puppis
2 R.A. Downes et al., 2001, PASP 113, 764 (2006 archival version) 2005JAD....11....2D
3 R.A. Downes et al., 2001, PASP 113, 764 2001PASP..113..764D
4 K.J.Meech, PASP 95, N571, 662, 1983. 1983PASP...95..662M
5 M.F.Walker, Bud Mitt N57, 1965=Lick Contr N179. 1965CoKon..57....1W
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Revision History
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3 Otero, Sebastian Alberto 2011-05-16 14:58 UTC Primary record creation. Variability type, spectral type and minimum magnitude from reference. UCAC3 position.
2 Admin, VSX 2010-01-04 23:43 UTC Position updated from the GCVS version of November 2009.
1 Admin, VSX 2005-12-17 20:33 UTC Initial upload.