... NED) which is operated by the Jet Propulsion Laboratory, Caltech, under contract ... 1 s RAsSN Right Ascension 1950 (seconds) 87 A1 --- DE-SN Declination 1950 (sign) 88 ...
... M V = \Gamma12, about three magnitudes brighter than the brightest open clusters in ... S.M. 1985, ApJ 299, 211 Ferguson A.M.N., Gallagher J.S., Wyse R.F.G. 1998, AJ 116 ...
... Located 9".4 west and 18".1 north of the center of UGC 4185 ( Discovery image ) ( JM Llapasset image ) ( JM Llapasset image ) ( Josep M. Bosch image ) ( Josep M. Bosch image ) . ...
... Located 44".3 east and 11".9 north of the nucleus of UGC 1394 ( Discovery image ( mirror ) ( local mirror )) ( Orbit Jet Obs image ) ( J. M. Llapasset image ) ( Rezman Obs image ) ( Campo Catino Obs image ) . ...
... Все звезды разбиты на спектральные классы от самых горячих к холодным: O, B, A, F, G, K, M. В частности, к классу O принадлежат голубые горячие звезды, к классу M - холодные красные. ...
... m s o ' " mm 770415 V4755 Sgr 17 44 51.7 -29 08 03 9.5 10.2 K M: 133 2MASS 770416 ... m s o ' " mm 770461 V4801 Sgr 17 45 08.0 -29 09 01 9.4 9.9 K M: 133 2MASS 770462 ...
... TU Cas M - m var (0.17P <= M - m <= 0.35P). TV Cas d = 0.01P. Min II 7.34. ... A var, M - m var (Pi = 0.2358d): DY Peg 0.55m < A < 0.67m, 0.24P < M - m < 0.42P ... m) ~0.1m in several minutes); irregular GK Per fluctuations from night to night ...