... 1997). The brightest O star Puppis (O4I(n)f ) is the most attractive target in searching for the magnetic field. ... Recently Chessneau & Moffat (2002) have reported a new attempt to detect the magnetic field in Puppis. ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/2003/2003_p250.pdf -- 444.9 Кб -- 21.04.2010
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Ссылки http://www.sao.ru/hq/lizm/conferences/pdf/2003/2003_p250.pdf -- 444.9 Кб -- 21.04.2010
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Ссылки http://jet.sao.ru/hq/lizm/conferences/pdf/2003/2003_p250.pdf -- 444.9 Кб -- 21.04.2010 Похожие документы
... 271 Table 1: The results of our calculations Star Puppis Ori Deneb P Cyg WR 40 T 0.2 0.17 0.03 1 3.4 Bl = 100 G Pl = 0.4% 0.17 ... The optical thickness of this wind is < 1 for Puppis and Deneb, and > 1 for P Cyg, WR 40 (Chesneau et al., 2003). ...
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Ссылки http://www.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p264.pdf -- 352.3 Кб -- 11.08.2011
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p264.pdf -- 352.3 Кб -- 11.08.2011 Похожие документы
... Society of New Zealand) containing various historic lists and catalogues of Galactic objects, namely: Dark Nebulae; Galactic OB Associations; LMC OB Stars; the Magellanic Clouds; the Orion Nebula Region; the Reed Areas (in Puppis); and the Sharov 5.3.2 ...
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Ссылки http://www.armaghplanet.com/pdf/Administration/MC-Mtg-2012-06-21-Final-2012-11-22.pdf -- 267.7 Кб -- 27.02.2013
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Ссылки http://star.arm.ac.uk/FOI/minutes/MC-Mtg-2012-06-21-Final-2012-11-22.pdf -- 267.7 Кб -- 25.01.2013 Похожие документы
... We highlight recent Chandra results on Cas A, Puppis A, E0102-72 and other remnants, touching on nucleosynthesis and mixing, velocity structure and equilibration processes.}, persons_number={0}, pdate={10Apr06 00:00:00}, date={24Apr06 18:35:03 ...