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Ссылки http://www.atnf.csiro.au/research/publications/ATNF_Publications_2009.pdf -- 85.2 Кб -- 03.03.2010 Похожие документы
... K., & Percival, J. W. 1998, PASA, 15, 14 Rodgers, A. W., Campbell, C. T., & Whiteoak, J. B. 1960, MNRAS, 121, 103 Russeil, D., Georgelin, Y. M., Amram, P., Georgelin, Y. P., Laval, A., & Marcelin, M. 1998, PASA, 15, 9 Acknowledgments It is a pleasure to ...
... v hel = 688 +- 3 km/s . w 50 = 71 km/s . w 20 = 103 km/s . v LG D h75 = 6.2 Mpc . log M HI (Msun) = 8.70 . ... w 50 = 71 km/s . w 20 = 103 km/s . v LG D h75 = 6.2 Mpc . log M HI (Msun) = 8.70 . Original: B. Koribalski (21-Feb-2005) . ...
... M Humphreys University of Minnesota VY CMa IRC +10420 NML Cyg The Cool Hypergiants -- lie just below the upper luminosity ... 103 G at the star (extrapolating from OH masers at several 1000 AU) IRC +10420 -- circular polarization of OH (Nedoluha ...
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Ссылки http://www.atnf.csiro.au/research/masermeeting/web_papers/503_RHumphreys.pdf -- 697.0 Кб -- 09.04.2007 Похожие документы
... We have chosen two models, both with metallicity Z /Z = 0.25 and 1 and with a total mass of 103 and 106 M . ... Castander, F. J. 2004, ApJ, 615, 689 Garnett, D. R. 1992, AJ, 103, 1330 Garnett, D. R., Shields, G. A., Peimbert, M., et al ...
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Ссылки http://www.atnf.csiro.au/people/Angel.Lopez-Sanchez/papers/LSEGR06.pdf -- 1792.2 Кб -- 02.02.2008 Похожие документы