... star as a conventional star with very high mass ( M = 103 -106 M ) (see also Shapiro ... masses of about 50 M , and is maintained until the end of their calculation at 103M ...
... Adopting this value, and T d = 30 K, we arrive at a 2 mass detection limit of Md 8.7 в 103M 2 . 2.2. ... carbon (Serra Diaz-CaЯo & Jones 2008)then d (250 m) = 1.932 (Rouleau & Martin 1991)and the mass detection limit Md 2.9 в 103M ...
... an average dust temperature of T d = 20 K, we convert this noise estimate to a 3 dust mass detection limit of Md = 2.44 в 103M ... 2003). Their Hi upper limit corresponds to a 3 dust mass limit of 8 в 103M , well below the SDP detection limit. ...
... we estimate a gas mass of about 1.1 в 103M in a region with a diameter of 0.32 pc ... 30-m telescope towards the HC position is 58 K km s-1 (in main beam temperature ...
... point. 5 with a mass in excess of 103M and a bolometric luminosity of 2в105 L (L ... from 5 в 102 M to 2 в 103M , depending on the statistical distribution of the stars ...
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Ссылки http://www.arcetri.astro.it/science/starform/preprints/mosca_06.pdf -- 1253.0 Кб -- 17.01.2012 Похожие документы
... in the same way as for 12 CO(1-0), amounting to Mgas (13 CO) = 1.2 в 103M ... showing detectable 13 CO(2-1) emission; we found Mgas (12 CO) = 4.8 в 103M ... 103 Rosolowsky, E., & Blitz, L. 2005, ApJ, 623, 826 Rosolowsky, E., Leroy, A. 2006 ...
... Per la riga larga H sono state ottenute larghezze comprese tra 1000 e 10000 km/s, con un valore medio di vH broad = (37.3 ± 1.6)102 k m/s e std = 2 103 k m/s, cio` i valori caratteristici delle larghezze e delle righe di emissione della BLR. ...
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Ссылки http://www.arcetri.astro.it/~marconi/TESI/TommasoPecchioli.pdf -- 2036.0 Кб -- 25.01.2012 Похожие документы
... et al. 2010) is translated into an average 5 upper dust mass limit Md 6 з 103M ... with the bulk of genuine ETGs with significantly lower dust masses ( 6 з 103M ... to the average upper dust mass limit in genuine early-type dwarfs (Md < 6 з 103M ...
... Results. Our observations resolve the HMC into three cores whose masses are on the order of 101 - 103M . ... cores in G 19.61-0.23 on the order of 101 103M one can hypothesize that each of them could develop an HII region; the ...
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Ссылки http://www.arcetri.astro.it/science/starform/preprints/cesa_21.pdf -- 1687.4 Кб -- 21.06.2010 Похожие документы