... Arumov G.P., Bukharin A.V., Perfil`eva I.M. 'Refinement of the Method for Determinating of the AngularSize of the Halo from the Plane Wave Passed Through a Statistically Inhomogeneous Screen'. ...
... This size is also consistent with the models of Jupiter formation, which require these rather large sizes of dust particles in order to obtain sufficiently low opacity, leading to the high accretion rate of the planet. ...
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Ссылки http://www.cosmos.ru/conf/2009elw/presentations/presentations_pdf/session4/Makalkin_ELW.pdf -- 340.2 Кб -- 20.04.2009 Похожие документы
... Arumov G.P., Bukharin A.V., Perfil`eva I.M. 'Refinement of the Method for Determinating of the AngularSize of the Halo from the Plane Wave Passed Through a Statistically Inhomogeneous Screen'. ...
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... of Technology in Haifa (Technion) in 1960, after completing a study of the angular distribution of cosmic ray muons underground ... He has produced a on the world-wide web three book-sized scientific overviews . ...
... of Technology in Haifa (Technion) in 1960, after completing a study of the angular distribution of cosmic ray muons underground ... He has produced a on the world-wide web three book-sized scientific overviews . ...
... of Technology in Haifa (Technion) in 1960, after completing a study of the angular distribution of cosmic ray muons underground ... He has produced a on the world-wide web three book-sized scientific overviews . ...