... DDR B. Musielok Astronomical Institute, Wroclaw University Kopernika, 11, 51-622, Wroclaw, Poland ABSTRACT The Ap star HB 152107 (=BS 6254 = 52 Her) is one of the small number of magnetic CP stars with long time or long periodic variability ...
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Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1987/1987_p79-p80.pdf -- 20.5 Кб -- 24.02.2010 Похожие документы
... The derived radial velocity of the star is km/s. The star HD 5797=V55 1 Cas is a less known CP2 star. ... Adelman (1973) included this star in the well-known list of 21 cool sharp-lined Ap stars. ...
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Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/1987/1987_p56-p58.pdf -- 32.3 Кб -- 24.02.2010 Похожие документы
... International Conference "Physics and Evolution of Magnetic and Related Stars" . Special Astrophysical Observatory, Russia . ... Fax: . +7 (87878) 4 65 27 (marked "Magnetic Stars-2014") . E-mail: . ? Iosif I. Romanyuk, Chair of Organizing Committee. ...
... Jets from young stellar objects . Velocities of stars in globular clusters. ... for which the image of the circumnuclear star formation ring in Ha with lines of ... of the absorption line we have measured radial velocities more than 700 stars ...
... stars (hereafter also referred to as proto-planetary nebulae - PPNe) being in the transition phase from AGB to planetary nebulae offer an opportunity to study in detail a chemical composition which has undergone changes due to nucleosynthesis and mixing ...
... Panchuk V.E. Some physical properties of the shock-waves in the RR Lyraes stars atmospheres. ... In: "Problems of space physics", Naukova Dumka, Kiev, 1971, iss.6, p.199-204. Panchuk V.E. On the convection in M-stars. Sov. ...
... Searc h for magneti c star s amon g youn g Herbi g Ae/B e star s Yu.V . ... star s turne d ou t t o b e chemicall y peculia r magneti c He-ric h an d He-wea k ... star s ther e appeare d t o b e no t a singl e chemicall y peculia r sta r o f th e ...
... star IRC+10 216: A high spatial-resolution time sequence of dust-shell evolution G. Weigelt, T. Blocker, K.-H. Hofmann, A. Men'shchikov, J.M. Winters Max{Planck{Institut fur Radioastronomie, 53121 Bonn, Germany Y. Balega Special Astrophysical ...
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Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2002/WBBHMW_2002.ps -- 260.3 Кб -- 24.02.2010 Похожие документы
... The star became invisible in U band frames. ... two nights we have accumulated 6000 s exposures to get measurable image of the star ... V838 Mon was a system containing two B3V type stars, and brighter companion exploded ...