... дб # е й$ # 16:30-17:00 .. , , .. ( .. , ", ) 30 ) 30 30 ) d 17:00-17:30 йp on m17:30-18:00 .. ( ), . 30 . ... i Uv i дг Q# v# ж ( d дж вг д й! д де д# # x е 7 d k 16:30-17:00 .. ,.. ( 30 - д ж d г е д ж 17:00-17:30 qp йp on m17:30-18:00 ...
... For the highest expected background level, i.e., within the Galactic Plane and with largest zodiacal light, the limiting magnitude will be below m(V) 17.4 (also for 5000 s effective integration). ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/J31_Mas-Hesse01-14Jun07_18:37:37.pdf -- 759.1 Кб -- 14.06.2007 Похожие документы
... A&A 411, L261, 2003. [17] Miller J.M., Raymond J., Fabian A.C. et al., ApJ 601, 450, 2004. [18] Morrison R. and McCammon D., ApJ 270, 119, 1983. ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/G30_Balman01-05Mar07_11:54:53.pdf -- 149.1 Кб -- 05.03.2007 Похожие документы
... of extinction as well as stellar density, and non-unique connection between mass and spectral type, and draws attention to the fact that one would have to include B3 dwarfs as well, if the lower mass limit for supernovae is 8 M instead of 10 M (e.g., [17 ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/B07_Hartmann01-07May07_12:04:00.pdf -- 279.4 Кб -- 07.05.2007 Похожие документы
... Durban), 237 [16] Bussard, R.W., Ramaty, R., and Drachman, R.J. 1979, ApJ, 228, 928 [17] Casse, M., Cordier, B., Paul, J., and Schanne, S. 2004, ApJ, 602, L17 [18] Cesarsky, C. J., and Voelk, H. J. 1978, A&A, 70, 367 [19] Chan, K.-W., and Lingenfelter, R ...
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Ссылки http://hea.iki.rssi.ru/integral06/papers/A06_Dogiel01-05Apr07_00:55:03.pdf -- 130.8 Кб -- 04.04.2007 Похожие документы