2004MNRAS.349.1505B

Query : 2004MNRAS.349.1505B

2004MNRAS.349.1505B - Mon. Not. R. Astron. Soc., 349, 1505-1508 (2004/April-3)

Mass-transfer bursts and the superhumps in cataclysmic variables.

BATH G.T.

Abstract (from CDS):

It is suggested that the superhumps in SU UMa stars are generated by a bright region on the red component that rotates asynchronously with the binary period. The bright region would be produced by mass-transfer instability by the red component. A simple experimental illustration of dynamical instability is presented, together with estimates of cooling times after instability.

Abstract Copyright: 2004 RAS

Journal keyword(s): instabilities - binaries: close - stars: dwarf novae - stars: mass-loss - novae, cataclysmic variables

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* Z Cha CV* 08 07 27.7517751528 -76 32 00.665029356           M5.5 620 1
2 V* DV UMa CV* 09 46 36.5964360384 +44 46 44.683031784   19.0       DA:+M 131 0
3 V* IY UMa CV* 10 43 56.7487980888 +58 07 31.920814488   17.52 16.61 17.62 17.60 ~ 119 0
4 V* WZ Sge CV* 20 07 36.5037622512 +17 42 14.733254952   15.30 15.20 10.817   D 982 0

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