... Recombination H110 alpha line in the OrionNebula . (1992) . ... wave length 6.2cm in the OrionNebula was obtained with the radiotelescope RATAN-600 ... Figure 1. Profiles of H110 alpha line in a central part of OrionNebula. ...
... line were observed in the region of OrionNebula with angular resolution of 2 ' x 20 ... On the hight of OrionNebula such sources were 3C 218 ( F = 37.4 J ) and 3C 273 ( F ...
... line were observed in the region of OrionNebula with angular resolution of 2 ' x 20 ... On the hight of OrionNebula such sources were 3C 218 ( F = 37.4 J ) and 3C 273 ( F ...
... magnetic fields in the massive stars of the OrionNebula Cluster V. Petit 1 1,2 , G ... and most massive memb er of the OrionNebula Cluster (ONC), and HD 191612 (Donati et ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2006/p218.pdf -- 147.8 Кб -- 26.12.2008 Похожие документы
... found for the low-mass stars in the OrionNebula cluster as well as in the field ... Introduction The OrionNebula cluster is one of the most prominent and nearby (D 450 ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_1999/1999A&A_347L_15W.pdf -- 242.6 Кб -- 05.08.2004 Похожие документы
... H. Multiplicity of the young O- and B-type stars in the OrionNebula cluster ... of the massive stars in the OrionNebula cluster and implications on their formation ... G., Zinnecker H. Multiplicity of the massive stars in the OrionNebula cluster ...
... The OrionNebula is one of the most prominent and nearest (D 450 pc) star forming ... survey for multiple systems among 13 O- and B-type OrionNebula cluster members ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2003/2003A&A_402_67S.pdf -- 204.3 Кб -- 01.02.2005 Похожие документы
... OB stars at the core of the OrionNebula Cluster, and it represents a perfect ... Introduction The OrionNebula (M42) is one of the closest (d 400-450 pc) and most ... Stauffer 1994; Hillenbrand 1997), which is known as the OrionNebula Cluster (ONC ...
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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