... astro-ph . ... SAI VO . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . Normalized to: Rucinski, S. 147 article(s) in total . 305 co-authors, from 1 to 69 common article(s). ... Cameron, A. Collier. Cameron, Chris. ... Charbonneau, David. ... David-Uraz, Alexandre. ... Eversberg, Thomas. Fabrycky, Daniel. ... Gordon, K. D.. ... Guenther, B. D.. Guenther, David B.. ... Huber, Daniel. ... Szentgyorgyi, Andrew H.. ...

. Found 4 documents . 2 декабря 2011 (Liakos, Niarchos) Discovery of Three New W UMa Stars . 18 апреля 2011 (Liakos, Niarchos) Discovery of Three W UMa Type Eclipsing Binaries . 30 ноября 2010 (Liakos, Niarchos) Discovery of Four New Variables . 18 февраля 2010 (Liakos, Niarchos) Photometric Elements for Five Newly Discovered Variable Stars .

... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

... SAI Crimean Station. ... ShV,f79: V.P.Goranskij, E.A.Karitskaya,A.V.Kusakin, S.Yu.Shugarov with photoelectric UBV photometer by S.Shugarov and I.Volkov (Red - reduced observations in non-linear counting regime; f79-the same photometer with f79 photomultiplier in BVR mode. 70-cm telescope of SAI Moscow Observatory; 60-cm and 125-cm telescopes of SAI Crimean Station, Ukraine; 38-cm telescope of Crimean Astrophysical Observatory, Ukraine; 60-cm telescope of INASAN Zvenigorod Station in the Moscow...

... 86 ­ 103 A Different Lo ok at Co ol Contact Binaries Stepien K. ё ґ Warsaw University Observatory, Warsaw, Poland Abstract. ... It assumes that W UMa­type stars are old ob jects which have passed the mass transfer episode with the mass ratio reversal. ... It is shown that the lack of hydrostatic equilibrium in a common envelope of the contact binary results in a large­scale flow of matter from the more massive primary to the secondary. ... The more massive, primary component is a MS star. ...

... Hour of right ascension (alpha, h), B1950.0 6. ... Degree of declination (delta, deg), B1950.0 9. ... Unsertainty in Delta(delta), arcsec --------------------------------------------------------------------------------------------- Year alpha delta alpha delta Unsertainties N month B1950.0 B1950.0 J2000.0 J2000.0 D(alpha) D(delta) sat day h m s deg ' '' h m s deg ' '' cos(delta) with decimals arcsec arcsec --------------------------------------------------------------------------------------------- ...

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... Star Atlas . ... Study yields new variable stars . ... The study hopes to shed light on how a wide variety of stars vary over many years by monitoring the luminosity stability of normal stars, searching for changes in the periods and amplitudes of variable stars, and waiting for any flares or outbursts. ... If these contact binaries prove to be members of the star cluster instead of foreground or background stars, Wilkerson said, they will be useful as part of a study of how the systems evolve. ...