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Contact binaries and multiple systems

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Dissertation

Photometric and spectroscopic research of the contact binary system AW UMa (in Slovak language)

Abstract

The main goal of this thesis was to determine basic characteristics of the components of AW UMa contact binary and find the cause of the light curve and orbital period changes. Another aim of the work was to prove or disaprove possible existence of the third body and to found simple but consistent model of the system. The investigation presented in this work was based on a large photometric and spectroscopic material obtained partly by the author and his supervisor. The most important results of the work are: Basic characteristics of the components of the quadrupole system AW UMa were found. Masses of the components of the contact system set AW UMa on the Zero Age Main Sequence.

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Submitted papers:

T. Pribulla, J.M. Kreiner, J. Tremko: "Catalogue of the field contact binary stars" (sumbitted to CAOSP)


Abstract:

The catalogue of 361 galactic contact binaries is presented. Enlisted contact binaries are divided into five groups according to the type and quality of the available observations and parameters. For all systems the ephemeris for the primary minimum, minimum and maximum visual brightness and equatorial coordinates are given. If available, photometric elements, $(m_1 + m_2) \sin^3 i$, spectral type, parallax and magnitude of the O'Connell effect are also given. Photometric data for several systems are augmented by new observations. The quality of the available data is assessed and systems requiring modern light-curve solutions are selected. Selected statistical properties of the collected data are discussed.

Postscript version of the paper


Last modified: November 18, 2002

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