... 5007) / F(H) a Salpeter IMF, a total mass of 106M and a 100 M upper stellar mass ... We obtain T D = 43.2K and MD = 7.62 в 106M . ... Moles, M., & Masegosa, J. 1993, AJ, 106, 1784 Castellanos, M. 2000, Ph.D. Thesis: A ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/papers/LSER04b.pdf -- 1035.6 Кб -- 02.02.2008 Похожие документы
... burst with a Salpeter IMF, a total mass of 106M and a 100 M upper mass, but with ... We have considered a 106M instantaneous burst and three different stellar mass ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/papers/LSER04a.pdf -- 1151.2 Кб -- 02.02.2008 Похожие документы
... The most massive (M 25 M for Z ) luminous (105 to 106 L ) and hot (temperatures 50 000 K) O stars evolve to the Wolf-Rayet ... mass created a in the starburst (a normalization factor) was set to 1 M and 106M for SV98 and SB99 models, respectively ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/papers/MSFinWRG_III_29apr09_editors.pdf -- 752.5 Кб -- 30.04.2010 Похожие документы
... shallow survey discussed here consists of two scans in longitude separated by b = 17 arcmin, resulting in an rms noise of about 15 mJy, equivalent to a 5 HI mass detection limit of 4 в 106 d2 c M (for a galaxy Mp with the typical linewidth of 200 km s-1 ...
... References Bertelli, G., Bressan, A., Chiosi, C., Fagotto, F., & Nasi, E. 1994, A&AS, 106, 275 Bessell, M. S. 1993, in Precision Photometry, ed. D. Kilkenny et al. ...