papers

Publications (10)

astro-ph.SR2014

HD 183648: a Kepler eclipsing binary with anomalous ellipsoidal variations and a pulsating component

T. Borkovits, A. Derekas, J. Fuller +16

KIC 8560861 (HD 183648) is a marginally eccentric (e=0.05) eclipsing binary with an orbital period of P_orb=31.973d, exhibiting mmag amplitude pulsations on time scales of a few da…

astro-ph.SR2014

Modelling of Sigma Scorpii, a high-mass binary with a Beta Cep variable primary component

A. Tkachenko, C. Aerts, K. Pavlovski +6

High-mass binary stars are known to show an unexplained discrepancy between the dynamical masses of the individual components and those predicted by models. In this work, we study…

astro-ph.SR2015

Spectroscopically resolving the Algol triple system

V. Kolbas, K. Pavlovski, J. Southworth +7

Algol ( Persei) is the prototypical semi-detached eclipsing binary and a hierarchical triple system. From 2006 to 2010 we obtained 121 high-resolution and high-S/N échelle spe…

astro-ph.SR2016

Stellar modelling of Spica, a high-mass spectroscopic binary with a beta Cep variable primary component

A. Tkachenko, J. M. Matthews, C. Aerts +16

Binary stars provide a valuable test of stellar structure and evolution, because the masses of the individual stellar components can be derived with high accuracy and in a model-in…

astro-ph.SR2013

Absolute dimensions of detached eclipsing binaries. III. The metallic-lined system YZ Cassiopeiae

K. Pavlovski, J. Southworth, V. Kolbas +1

The bright binary system YZ Cassiopeiae is a remarkable laboratory for studying the Am phenomenon. It consists of a metallic-lined A2 star and an F2 dwarf on a circular orbit, whic…

astro-ph.SR2011

Apsidal motion of the eclipsing binary AS Camelopardalis: discrepancy resolved

K. Pavlovski, J. Southworth, V. Kolbas

We present a spectroscopic study of the eclipsing binary system AS Camelopardalis, the first such study based on phase-resolved CCD echelle spectra. Via a spectral disentangling an…

astro-ph.SR2013

The eccentric massive binary V380 Cyg: revised orbital elements and interpretation of the intrinsic variability of the primary component

A. Tkachenko, P. Degroote, C. Aerts +8

We present a detailed analysis and interpretation of the high-mass binary V380 Cyg, based on high-precision space photometry gathered with the Kepler space mission as well as high-…

astro-ph.SR2014

Tracing CNO exposed layers in the Algol-type binary system u Her

V. Kolbas, A. Dervisoglu, K. Pavlovski +1

The chemical composition of stellar photospheres in mass-transferring binary systems is a precious diagnostic of the nucleosynthesis processes that occur deep within stars, and pre…

astro-ph.SR2009

Chemical evolution of high-mass stars in close binaries. II. The evolved component of the eclipsing binary V380 Cygni

K. Pavlovski, E. Tamajo, P. Koubsky +3

The eclipsing and double-lined spectroscopic binary V380 Cyg is an extremely important probe of stellar evolution: its primary component is a high-mass star at the brink of leaving…

astro-ph.SR2010

Observational approach to the chemical evolution of high-mass binaries

K. Pavlovski, J. Southworth, E. Tamajo +1

The complexity of composite spectra of close binaries makes the study of the individual stellar spectra extremely difficult. For this reason there exists very little information on…