... study of magnetic fields in intermediate massstars A minimum field strength for Ap ... enough sample to study the evolution of Ap stars in the mass range between 2 and 5 M ...
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Ссылки http://star.arm.ac.uk/lectures/landstreet/text/landstreet-larochelle-3.pdf -- 742.9 Кб -- 07.02.2009 Похожие документы
... or radii, those which con tain white dwarf components and stars with masses 0.4M fi ... in convective turnover timescale for stars with mass differences of up to 0.5M fi ...
... globular cluster we were consists of two stars orbiting around their centre of mass, it enables investigating, we used the XMM ... I just registered a query the masses of stars to be calculated). ...
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Ссылки http://star.arm.ac.uk/~csj/nuffield/posters/Plunkett_2007.pdf -- 589.3 Кб -- 05.09.2007 Похожие документы
... and Sku manich (1972) suggested that lowmassstars arrive on the mainsequence ... yield information on the timescales for braking of progressively lower massstars ... the most comprehensive for the lowmassstars with which we are concerned here ...
... or, in the present case, the more massive helium star became a giant following core ... it would have originally been the more massivestar and that it would have lost its ...
... Telescope `FLAMES' Tarantula Survey that one of the most massivestars in the near Universe (the star VFTS 682, identified in ... PRESENTATION OF RESEARCH DR JORICK VINK THE MOST MASSIVESTARS IN THE UNIVERSE Dr Jorick Vink delivered a short ...
... INTRODUCTION Magnetism in hot, massivestars appears to be a relatively uncommon ... knowledge and scientific discussion regarding magnetism of pulsating massivestars ... Furthermore, the Magnetism in MassiveStars (MiMeS) survey component has found ...
... models of a 0.7 M mass helium star contracting towards the helium main-sequence ... Considerable mass is accumulated before the star leaves the yellow giant region. ...
... Low-massstars are formed in both types of cloud, but GMCs are the primary creation ... Since DCCs are the sites of low-massstars and close encounters with them are an ...
... on the theme of cool stars focused on the emerging field of very-low-massstars ... The second theme was the role of low-massstars in star formation. ... predict the ejection of many low-massstars and frequent disruption of their disks ...