... START END DESCRIPTION PROP-PROG:OB:AL VER -------------------------------------------------------------------------------- 104:11:23:45 D=00:00:06:15 * M Slew (AN= 0,RA=280,DE= 50,PA= 75,O= 0,SN= 90) 104:11:30:00 ******** Main SU POINTH1 ...
... Phillips, M. M. 1994, PASP, 106, 566 Hamuy, M., Walker, A. R., Suntzeff, N. B., Gigoux, P., Heathcote, S. R., & Phillips, M. M. 1992, PASP, 104, 533 Kaiser, M. E., et al. 2010, arXiv:1001.3925 Landolt, A. U., & Uomoto, A. K. 2007, AJ, 133, 768 Montegriffo ...
... appears to be no evidence for reddening for HD 181327 (unsurprising , given its distance and environment). pixelР1) with F110W (keA М 1:104m, FWHM М 0:5915 m) filter direct and coronagraphic imaging and supporting F180M (keA М 1:7968 m, FWHM М 0:0684 m ...
... PROG:OB:AL VER -------------------------------------------------------------------------------- 107:15:23:45 D=00:00:06:15 * M Slew (AN= 0,RA=224,DE=-15,PA=104,O= 2,SN=161) 107:15:30:00 ******** Main SU POINTH1 ******************************** 107:15:30 ...
... This rapid decline is seen for different mass ranges above 3 в 104M . ... C. 1994a, A & AS, 104, 365 Fagotto, F., Bressan, A., Bertelli, G., & Chiosi, C. 1994a, A & AS, 105, 29 Fall, S. M., 2004, in ...
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Ссылки http://www.stsci.edu/science/starburst/Preprints/Chandar_Diffuse.pdf -- 780.0 Кб -- 31.03.2005 Похожие документы