2009ApJ...703..109D


Query : 2009ApJ...703..109D

2009ApJ...703..109D - Astrophys. J., 703, 109-113 (2009/September-3)

Evidence of a brown dwarf in the eclipsing dwarf nova Z Chamaeleonis.

DAI Z., QIAN S. and FERNANDEZ LAJUS E.

Abstract (from CDS):

We presented three new CCD observations of light minima of Z Chamaeleonis. All 187 available times of light minimum including 37 photographic data are compiled, and a new orbital period analysis is made by means of the standard O - C technique. The O - C diagram of Z Chamaeleonis presents a cyclical periodic change of ∼ 32.57 yr with a high significance level. We attempted to apply two plausible mechanisms (i.e., Applegate's mechanism and light travel-time effect) to explain the cyclical variations of orbital period shown in the O-C diagram. Although the previous works suggested that solar-type magnetic cycles in the red dwarf are the best explanation, the analysis of Applegate's mechanism in this paper presents a negative result. Accordingly, a light travel-time effect is proposed, and a brown dwarf as a tertiary component orbiting around dwarf nova Z Chamaeleonis is derived with a significance level of ≳81.6%, which may be a plausible explanation of the periodic variation in the systemic velocity of Z Chamaeleonis in superoutburst.

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Journal keyword(s): binaries: eclipsing - novae, cataclysmic variables - stars: individual: Z Chamaeleonis

Simbad objects: 2

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Number of rows : 2
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* U Gem CV* 07 55 05.2324414746 +22 00 05.044127985   15.3 14.54     DA 1135 0
2 V* Z Cha CV* 08 07 27.7517751528 -76 32 00.665029356           M5.5 620 1

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