... Rotationallysupported circumstellar disks in the protostellar systems evidently originate in the collapse of selfgravitating, rotating molecularcloud cores. ...
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Ссылки http://www.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://www.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://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2006/p262.pdf -- 256.6 Кб -- 26.12.2008 Похожие документы
... dark cloud showing images from several positions within the dense molecular cores at ... the hyperlinked tour of the Lynds 1641 molecularcloud in Orion, and a library of ...
... 11:15 Coffee break . 11:45 J. Krelowski - Diffuse interstellar bands vs. rotational temperatures of simple molecular species . ... 11:30 General discussion on laboratory vs. theoretical spectra of molecular features . 12:00 Coffee break . ...
... Radio observations of K3-50A by Howard et al. (1997) revealed a attened cloud of dense molecular gas 1:1 pc in extent and a 0:5 pc inner torus. ...