... Вверху показан спектр звезды Romano, полученный в феврале 2006 (m v =17 m .27). ...
14. http://www.sao.ru/hq/lizm/conferences/pdf/2003/2003_p259.pdf
... References 5 1a, 1b, 2, 3, 4 14 m 17 b 8 6 b 27, 28 6 6 m 1a, 1b, 2, 3, 4, 18 14 1a, 1b, 2, 3, 12 2, 3 mb c 4, 5, 17, 22, 23 ...
15. Introduction
... Thus, the new Hamburg/SAO Survey (HSS) for emission-line galaxies leads, firstly, to the creation of a new BCG/H II galaxy sample in a large sky region with the boundaries 7 h 20 m to 17 h 40 m in right ascension and to in declination. ...
16. Introduction
... The boundaries of our survey are 7 h 20 m to 17 h 40 m in right ascension and to in declination, which bridges the gap between the zones of the Second Byurakan Survey (SBS; Markarian et al. ...
17. Introduction
... One of them includes 240 objects in the region of the SBS survey (Markarian et al. [ 1983 ], [ 1987 ]) = 7 h 40 m - 17 h 20 m , = within an area of about 1000 square degrees (Izotov et al. [ 1993a ], [ 1993b ], Pustilnik et al. [ 1995 ]) and is based on ...
18. Introduction
... It covers the region between 7 h 20 m to 17 h 40 m in right ascension and between to in declination. ...
19. http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2004/2004A&A_424_165.pdf
... T in 650-1200 K, 9.7 µm 7-17, and the silicate feature typically in absorption for ... sizes (see labels). is a0 = 0.17 µm, which should lead to a distribution comparable ...
20. ПРЕДИСЛОВИЕ
... Всего в сообщении содержится N1 букв типа А, N2 букв типа Б т.д. Общее число различных последовательностей из букв m-буквенного алфавита равно M формула (17) . ...