... well as isolated gas clouds or HVCs of a few times 106M. Westmeier et al., in prep ... H I masses typically 5 в 106M. Velocity dispersions of 10...20 km/s. H surveys with ...
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Ссылки http://www.atnf.csiro.au/research/WALLABY/Wallaby2010/TWestmeier-Wallaby2010.pdf -- 1945.9 Кб -- 08.12.2010 Похожие документы
... Those systems have HI masses around 106 - 108 M . ... imply a mass in excess of 106M , they discarded this possibility and suggested that ... Thompson, I., Roth, M., & Ruiz, M. T. 1993, AJ, 106, 1420 Mathewson, D., Cleary, M ...
... Comparison between Centaurus A and FR-I type RG 3C 31 Centaurus A Mdust ~ 106M sun ,T dust = 30-40 K (Leeuw & Eckart 2002) R(2-1)/(1-0) ~ 0.85-1.1 (Wild et al. ...
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Ссылки http://www.atnf.csiro.au/research/cena/documents/presentations/okuda.pdf -- 1509.2 Кб -- 16.07.2009 Похожие документы
... BL Lac M 87 106 107 108 109 109 106 107 (Cooling Flow ) (Low-M Merger ) 108 109 ... two gas-rich systems, the BH of the merging galaxies can grow from 106M to 109 M ...
... Bandwidth dep olarization: This dep olarization mechanism requires very high, homogeneous RM (106 rad m-2 ), and such conditions should also pro duce strong FFA which is not seen along most of the dep olarized jets. ...
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Ссылки http://www.atnf.csiro.au/people/Enno.Middelberg/pubs/middelberg2005b/middelberg2005b.pdf -- 92.6 Кб -- 02.06.2004 Похожие документы
... The total H luminosity of the galaxy indicates a total ionized mass of MH I I = (3.4 ± 0.2) в 106M and a star formation rate of S F RH = 1.82 ± 0.13 M a-1 . ...
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Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/proceedings/NOT_CONTRIBUTION_2006_lopez-sanchez.pdf -- 347.4 Кб -- 22.03.2007 Похожие документы