1999MNRAS.305..473L


Query : 1999MNRAS.305..473L

1999MNRAS.305..473L - Mon. Not. R. Astron. Soc., 305, 473-480 (1999/May-2)

WZ Sagittae as a DQ Herculis star.

LASOTA J.-P., KUULKERS E. and CHARLES P.

Abstract (from CDS):

We argue that quiescent WZ Sge is a rapidly spinning magnetic rotator in which most of the matter transferred from the secondary is ejected from the system. Assuming that the observed 27.87-s oscillation period results from the spinning white dwarf, we propose that the other observed principal period of 28.96 s is a beat caused by reprocessing of the rotating white dwarf beam on plasma blobs in Keplerian rotation at the outer disc rim. The weaker, transient, 29.69-s period is identified as a beat with the Keplerian period of the magnetosphere. WZ Sge evolves through a cycle of spin-up and spin-down phases. During the spin-down phase it is a DQ Her star; during the spin-up phase it should be a ER UMa star.

Abstract Copyright: 1999, Royal Astronomical Society

Journal keyword(s): stars: individual: WZ Sge - stars: magnetic fields novae, cataclysmic variables - stars: oscillations - stars: rotation

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* HT Cam CV* 07 57 01.3362559272 +63 06 02.000945340   16.36       ~ 78 0
2 V* V1025 Cen CV* 12 38 16.3191432264 -38 42 45.836441856   15.20       ~ 90 0
3 V* WZ Sge CV* 20 07 36.5037622512 +17 42 14.733254952   15.30 15.20 10.817   D 982 0
4 V* AE Aqr CV* 20 40 09.1598959176 -00 52 15.055595220   12.46 10.40   10.191 K3-5IV/V 705 0

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