... 0.005 µm and amax = 0.45 µm. The observed dust shell properties cannot be fitted by ... We chose Draine & Lee (1984) silicates with amin = 0.005 µm and amax = 0.45 µm. 3.4. ...
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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
... The absolute coordinates of IRS1 are # = 23 h 13 m45. s 35 and # = +61 # 28 # 10. ... Name RA (J2000) a DEC (J2000) a K' Magnitude b Comment a 23 h 13 m45. s 33 61 # 28 # 21. ## 02 10. m 94 b 44. s 81 10. ## 63 ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/kraus_etal_aua_ngc7538irs1.5_2006.ps -- 2399.0 Кб -- 05.05.2009 Похожие документы
... originating from stars with masses in the range of 8 M /M45, and predicted about 447 000 active pulsars in the Galaxy with ... the magnetic field distribution of the main sequence massive stars (8 45M ) predicted by Ferrario & Wickramasinghe (2006 ...
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Ссылки http://mavr.sao.ru/Doc-en/Science/Public/Conf/magstars-2010/p303.pdf -- 262.8 Кб -- 11.08.2011 Похожие документы
... As a ux density and coordinate standard we used the strong radio source 1245-197 (RA 1950:0 = 12 h 45m45: s 22, Dec 1950:0 = {19 ф 42 0 57: 00 5). ...
... 45, Nova Mus 1991 and XTE J1650500) with black hole masses that are only very ... Webb et al. (2000) concluded i < 45 and M > 2.2 M with a maximum ma Data for 32 X ... M. Reid, private communication. c Estimated range based on extreme values observed ...