1994A&A...288L...9H


Query : 1994A&A...288L...9H

1994A&A...288L...9H - Astronomy and Astrophysics, volume 288L9-12 (1994/8-1)

Empirical masses and radii for the luminous binary Sk-67 105 in the LMC.

HAEFNER R., SIMON K.P. and FIEDLER A.

Abstract (from CDS):

The detection of optical light variability of Sk-67 105, one of the most massive binaries in the LMC, enables in combination with known spectroscopic data the determination of empirical masses and radii of the components using a light curve synthesis program. It is found that the system is nearly in contact and presumedly passes through Case A mass transfer at the moment. The derived pseudoeccentricity of the orbit may be explained by non-uniform brightness distribution within the system.

Abstract Copyright: ∼

Journal keyword(s): stars: early-type - stars: fundamental parameters - stars: individual: Sk -67 105 - binaries: spectroscopic - binaries: eclipsing - galaxies: Magellanic Clouds

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 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
3 SK -67 105 SB* 05 26 06.1884853848 -67 10 56.784543384 11.785 12.27 12.42   11.661 OB 46 0

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