... 2003). Other geometries have also been discussed, such as an extended disk or torus consisting of several molecularclouds (e.g., Cameron et al. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2004/2004A&A_425_77.pdf -- 483.6 Кб -- 01.02.2005 Похожие документы
... For the radial velocity of the center of mass, we determine 23.6 km s-1 , which is in good agreement with the heliocentric velocity of the Orion MolecularCloud (28 km s-1 , O'Dell 2001). ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2009/2009A&A...497..195K.pdf -- 1563.5 Кб -- 18.05.2009 Похожие документы
... Rotationallysupported circumstellar disks in the protostellar systems evidently originate in the collapse of selfgravitating, rotating molecularcloud cores. ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p061.pdf -- 374.0 Кб -- 11.08.2011 Похожие документы
... The results of the radial velocity study of Stahl et al. (2008) indicate that this star is rapidly moving away from the Orion MolecularCloud and its host cluster. ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p157.pdf -- 115.5 Кб -- 11.08.2011 Похожие документы
... It means, that the field is a dynamically stable relic of the field in the molecularcloud where the star formed, or of a field built by a dynamo acting in a pre-main sequence phase of the star (Mestel 2003). ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2006/p262.pdf -- 256.6 Кб -- 26.12.2008 Похожие документы