Bibcode
Szalai, T.; Kiss, L. L.; Mészáros, Sz.; Vinkó, J.; Csizmadia, Sz.
Referencia bibliográfica
Astronomy and Astrophysics, Volume 465, Issue 3, April III 2007, pp.943-952
Fecha de publicación:
4
2007
Revista
Número de citas
50
Número de citas referidas
47
Descripción
Aims:We detected tertiary components of close binaries from spectroscopy
and light curve modelling, investigated the light-travel time effect and
the possibility of magnetic activity cycles, measured mass ratios for
unstudied systems, and derived absolute parameters. Methods: We
carried out new photometric and spectroscopic observations of five
bright (< V >< 10.5 mag) close eclipsing binaries,
predominantly in the southern skies. We obtained full Johnson BV light
curves, which were modelled with the Wilson-Devinney code. Radial
velocities were measured with the cross-correlation method using IAU
radial velocity standards as spectral templates. Period changes were
studied with the O-C method, utilising published epochs of minimum light
(XY Leo) and ASAS photometry (VZ Lib). Results: For three
objects (DX Tuc, QY Hya, V870 Ara), absolute parameters have been
determined for the first time. We spectroscopically detected the
tertiary components in XY Leo and VZ Lib and discovered one in QY Hya.
For XY Leo we updated the light-time effect parameters and detected a
secondary periodicity of about 5100 d in the O-C diagram that may hint
at the existence of short-period magnetic cycles. A combination of
recent photometric data shows that the orbital period of the tertiary
star in VZ Lib is likely to be over 1500 d. QY Hya is a semi-detached
X-ray active binary in a triple system with K and M-type components,
while V870 Ara is a contact binary with the third smallest spectroscopic
mass ratio for a W UMa star to date (q = 0.082 ± 0.030). Being
close to the theoretical minimum for contact binaries, this small mass
ratio suggests that V870 Ara has the potential of constraining
evolutionary scenarios of binary mergers. The inferred distances to
these systems are compatible with the Hipparcos parallaxes.
Based on observations made at the Siding Spring Observatory, Australia.
Light curves and radial velocity data are only available in electronic
form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5)
or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/465/943