... of the star, M -- mass of the main comp onent of the system, M -- mass loss rate, L ... 6-m telescop e (Kholtygin et al. 2006c , sp ectrograph NES) and also in Bohyunsan ...
23. http://www.astro.spbu.ru/staff/ilin2/INTAS2/PAP/P6_4.pdf
... Fulle, M., Mikuz, H., Nonino, M., and Bosio, S.: 1998, Icarus 134, 235248. ... Harris, W. M., Combi, M. R., Honeycutt, R. K., Mueller, B. E. A., and Scherb, F.: 1997, Science 277, 676681. ...
24. Database of Optical Constants -- Level: group of materials
... 4.3, 15.1 bands . Palumbo et al. (1998) Astron. Astrophys. 334, 247. a m m o n i a i c e . NH 3 . abs. 0.2 - 1 . ...
25. http://www.astro.spbu.ru/DOP/8-GLIB/op3/JQSRT_110_1356.pdf
... M z ?r о? b1 lm ?iо ;lm M r ?r оо; lm r 2 Di , (10) where the vector wave functions ... for different m independently, and hereafter we skip the index m. So, for each m one ...
26. Bibliography
... 252 . Heller W., Tibibian R.M., Nakagaki M., Papazian L. Flow light scattering. 1. ... Mishchenko M.I., Dlugach J.M., Yanovitskij E.G. Multiple light scattering by ...
27. http://www.astro.spbu.ru/staff/ilin2/INTAS2/PAP/P6_1.pdf
... R. Astron. Soc. 250, 654 656. Festou, M. G., G. P. Tozzi, L. A. Smaldone, P. Felenbok, R. Falciani, and J.-M. Zucconi 1990. ...
28. http://www.astro.spbu.ru/Sobolev100/sites/default/files/Sobolev-100.pdf
... objects: classics today Sobolev-100 Conference, St.Petersburg State University, 2015 106 Interstellar p olarization and star formation studies in dark clouds A. Sen, M. Prokop jeva, V. Il'in , N. Voshchinnikov, R. Gupta Assam University, India asokesen ...
29. http://www.astro.spbu.ru/staff/ilin2/INTAS/P3-SPB1/PUBL/TEXT/vs-pazh.pdf
... and oblate spheroidal (a/b = 4) and spherical amorphous carbon (AC1) grains with rV = 0.01 µm at R = 104 R from the star ... The sphere temperature is Td(sphere) = 10.5, 20.4, 63.1, 106.4, and 226.4 K for T = 500, 1000, 3000, 5000, and 10 000 K ...
30. Symbols
... J . K . L . M . N . O . P . ... 103; . h . i . j . k . l . m . ...