UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 Cyg

ABSTRACT. Analysis of the polarimetric measurements of the eclipsing binary system V448 Cyg in wide UBVRI niters has shown the presence of the following components of the polarization: a) interstellar; b) constant intrinsic polarization with a flat spectrum; c) phase-dependent contribution, the ampl...

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Main Authors: N. M. Shakhovskoy, G. V. Volkova, Yu. L. Manilov, N. H. Minikulov
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2017-08-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/98779
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author N. M. Shakhovskoy
G. V. Volkova
Yu. L. Manilov
N. H. Minikulov
author_facet N. M. Shakhovskoy
G. V. Volkova
Yu. L. Manilov
N. H. Minikulov
author_sort N. M. Shakhovskoy
collection DOAJ
description ABSTRACT. Analysis of the polarimetric measurements of the eclipsing binary system V448 Cyg in wide UBVRI niters has shown the presence of the following components of the polarization: a) interstellar; b) constant intrinsic polarization with a flat spectrum; c) phase-dependent contribution, the amplitude of which decreases with wavelength. Constant component is possibly caused by an extended disk-like optically thin refracting envelope; the variable one may be caused by relatively dense condensations near the Lagrangian points in a binary. By analyzing the Fourier harmonics, the inclination angle is found to be i = 82°. The orbital plane of the system is inclined in respect to the Galaxy plane at an angle 70°. Mass of the extended envelope is estimated to be 1.5 x 10-8 M☉ with a mass loss rate 8.6 x 10-7 M☉/yr. Key words: Stars: binaries: close, eclipsing; circumstellar matter; polarization.
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spelling doaj.art-7633e943e3454aceb2b7dfca29be71342022-12-22T01:19:52ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-08-017110.18524/1810-4215.1994.7.9877998779UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 CygN. M. Shakhovskoy0G. V. VolkovaYu. L. ManilovN. H. MinikulovDepartment of Astronomy and Astronomical Observatory, Odessa National University, Odessa 65014 UkraineABSTRACT. Analysis of the polarimetric measurements of the eclipsing binary system V448 Cyg in wide UBVRI niters has shown the presence of the following components of the polarization: a) interstellar; b) constant intrinsic polarization with a flat spectrum; c) phase-dependent contribution, the amplitude of which decreases with wavelength. Constant component is possibly caused by an extended disk-like optically thin refracting envelope; the variable one may be caused by relatively dense condensations near the Lagrangian points in a binary. By analyzing the Fourier harmonics, the inclination angle is found to be i = 82°. The orbital plane of the system is inclined in respect to the Galaxy plane at an angle 70°. Mass of the extended envelope is estimated to be 1.5 x 10-8 M☉ with a mass loss rate 8.6 x 10-7 M☉/yr. Key words: Stars: binaries: close, eclipsing; circumstellar matter; polarization.http://oap.onu.edu.ua/article/view/98779
spellingShingle N. M. Shakhovskoy
G. V. Volkova
Yu. L. Manilov
N. H. Minikulov
UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 Cyg
Odessa Astronomical Publications
title UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 Cyg
title_full UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 Cyg
title_fullStr UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 Cyg
title_full_unstemmed UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 Cyg
title_short UBVRI POLARIMETRY OF CLOSE BINARY SYSTEM V448 Cyg
title_sort ubvri polarimetry of close binary system v448 cyg
url http://oap.onu.edu.ua/article/view/98779
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