... An Outbursting Protostar of the FU Orionis type in the Cygnus OB7 MolecularCloud" . ... An FU Orionis Outburst Object in the Cygnus OB7 MolecularCloud" . Movsessian T.A., Magakian T.Yu., ...
... The rise of CR flux and ultraviolet intensity is caused by the supernova bursts and by formation of massive OB stars, occurring in the giant molecularclouds. ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/1987/1987_p127-p131.pdf -- 48.7 Кб -- 24.02.2010 Похожие документы
... We present bispectrum speckle interferometry and speckle polarimetry of the deeply embedded infrared bipolar outflow source S140 IRS1, a massive protostellar object in the L1204 molecularcloud. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2000/2000A&A_361L_29S.pdf -- 286.3 Кб -- 03.08.2004 Похожие документы
... 2001AGM....18..P22P We explore the structures immediately surrounding the high-mass young stellar object S140 IRS 3 within the L1204 molecularcloud. ...
... P06P We present bispectrum speckle interferometry and speckle polarimetry of the deeply embedded infrared bipolar outflow source S140 IRS1, a massive protostellar object in the L1204 molecularcloud. ...
... If these fields result from (very approximate) flux freezing during star formation, from the giant molecularcloud phase up to the pre-main sequence, so that the magnetic flux mag R2 B (n0 /n)2/3 B is roughly constant, a field of 10-6 G at 103 particles ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/2003/2003_p11.pdf -- 110.4 Кб -- 21.04.2010 Похожие документы
... With this unusual structure which is likely to be of tidal origin (Makarova et al. 2003), neutral hydrogen filament and molecularclouds are associated ( Yun et al. ...