... Further observations were performed from the 1.5m RussianTurkish telescope, in TBITAK National Observatory, the 4.0 m Blanco ... Finally, 8 months after the burst, deep observations were made from the 3.5m telescope at Calar Alto. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2007/A&A_462_L57.ps -- 942.0 Кб -- 05.05.2009 Похожие документы
... 25.4 AU, an optical depth 2.2 µm = 6.5 ± 0.3, and dust grain radii ranging from amin ... A mass-loss rate of M = 5.58 в 105 M /yr was derived by Heske et al. (1990). ... for D = 2.30 kpc, ve = 15.1 km s-1 , 2.2 µm = 1.12, and M = 3.87 в 10-5M /yr ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2004/2004A&A_424_165.pdf -- 1961.2 Кб -- 01.02.2005 Похожие документы
... Using the relation AV /9.7 µm 21.5 (Schutte et al. 1998), an extinction of AV 15 can ... array, 2562 pixels, sensitivity from 1 to 2.5 µm, frame rate 2 frames/s) through an ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_229Y.pdf -- 168.2 Кб -- 03.08.2004 Похожие документы
... mass-loss rate can be determined to be M = (1.3-2.1) в 10-5M /yr for d = 500-800 pc ... 3 is eroded by strong stellar winds with current mass-loss rates close to 10-5M /yr ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2001/2001A&A_379_529H.pdf -- 322.5 Кб -- 03.08.2004 Похожие документы
... 3. Model SED for Teff = 7000 K, 0.55 µm = 5 and different dust temperatures T1 . ... underestimating the flux between 2 and 5 µm. Instead this part of the SED seems to ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_1999/1999A&A_348_805B.pdf -- 387.4 Кб -- 05.08.2004 Похожие документы
... Eq u ( v sin i < 5 k m s ) an d 4 9 Ca m ( v sin % = 2 2 k m s Th e typica l FOp ... n R V an d th e valu e 1.4 1.5 k m s fro m Wilson' s Genera l Catalo g o f Radia l ...
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Ссылки http://mavr.sao.ru/hq/lizm/conferences/pdf/1996/1996_p114.pdf -- 48.1 Кб -- 21.04.2010 Похожие документы