LONG-TERM PHOTOMETRIC AND SPECTROSCOPIC OBSERVATIONS OF THE NEAR-CONTACT BINARY KR CYGNI

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1. Verfasser: E. Sipahi
Format: Artículo científico
Sprache:en
Veröffentlicht: Universidad Nacional Autónoma de México 2013
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author E. Sipahi
author_facet E. Sipahi
contents LONG-TERM PHOTOMETRIC AND SPECTROSCOPIC OBSERVATIONS OF THE NEAR-CONTACT BINARY KR CYGNI E. Sipahi C. Ibanoĝlu Ö. Cakırlı Física, Astronomía y Matemáticas AKCMi DOCas) Binaries: close binaries: general binaries: eclipsing We present the multi-color, five-year light curves and the radial velocities of the near-contact binary system KR Cyg. We derived the masses of the components as 2.88 ± 0.20 M⊙ and 1.26 ± 0.07 M⊙ and the radii as 2.59 ± 0.06 R⊙ and 1.80 ± 0.04 R⊙. We also searched for the empirical determination of albedo and effective temperature of the cooler, less massive star of KRCyg, and of two similar near contact binaries AKCMi, and DOCas. The residuals between the observed and computed fluxes are attributed to the effect of mutual illumination which heats the surface layers of the illuminated star and does vary not only its bolometric albedo but also its limb-darkening coefficient and gravity-brightening exponent. The effective albedos are generally smaller than that expected from an envelope of convective star. These results are preliminary and speculative. 2013 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57126152003 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.1 Vol.49
format Artículo científico
id redalyc_57126152003
institution Redalyc
language en
publishDate 2013
publisher Universidad Nacional Autónoma de México
spellingShingle LONG-TERM PHOTOMETRIC AND SPECTROSCOPIC OBSERVATIONS OF THE NEAR-CONTACT BINARY KR CYGNI
E. Sipahi
Física, Astronomía y Matemáticas
AKCMi
DOCas)
Binaries: close
binaries: general
binaries: eclipsing
LONG-TERM PHOTOMETRIC AND SPECTROSCOPIC OBSERVATIONS OF THE NEAR-CONTACT BINARY KR CYGNI E. Sipahi C. Ibanoĝlu Ö. Cakırlı Física, Astronomía y Matemáticas AKCMi DOCas) Binaries: close binaries: general binaries: eclipsing We present the multi-color, five-year light curves and the radial velocities of the near-contact binary system KR Cyg. We derived the masses of the components as 2.88 ± 0.20 M⊙ and 1.26 ± 0.07 M⊙ and the radii as 2.59 ± 0.06 R⊙ and 1.80 ± 0.04 R⊙. We also searched for the empirical determination of albedo and effective temperature of the cooler, less massive star of KRCyg, and of two similar near contact binaries AKCMi, and DOCas. The residuals between the observed and computed fluxes are attributed to the effect of mutual illumination which heats the surface layers of the illuminated star and does vary not only its bolometric albedo but also its limb-darkening coefficient and gravity-brightening exponent. The effective albedos are generally smaller than that expected from an envelope of convective star. These results are preliminary and speculative. 2013 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57126152003 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Num.1 Vol.49
title LONG-TERM PHOTOMETRIC AND SPECTROSCOPIC OBSERVATIONS OF THE NEAR-CONTACT BINARY KR CYGNI
topic Física, Astronomía y Matemáticas
AKCMi
DOCas)
Binaries: close
binaries: general
binaries: eclipsing
url https://www.redalyc.org/articulo.oa?id=57126152003