... 322, L29 ± L36 (2001) The 2dF QSO Redshift Survey ± V. The 10k catalogue S. M. Croom,1w R. J. Smith,2 B. J. Boyle,1 T. Shanks,3 N. S. Loaring,4 L. Miller4 and I. J. Lewis1 1 2 3 4 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD Department of Physics, University of Durham, South Road, Durham DH1 3LE Department of Physics, Oxford University, 1 Keble Road, Oxford OX1 3RH Accepted 2001 March 7....

Download Izmccd (~2.7 MB). ... If you want to calculate equatorial coordinates of object: . Click the " File " menu, and then click " Open " ; or press  on toolbar. Choose a file with image. ... Also see section " Viewing of image ". ... Before, if it is necessary, you must make an account dark current and flat field (See section " Preliminary processing of images ".) ... Measure the marked stars. ... Click the " Calculations " menu, and then click " Coordinates " or . ...

... ОТЧЕТЫ СТУДЕНТОВ О ПРАКТИКЕ В САО . Лето 2002 года . ... Михаила Баринова . ... Исследование собственного движения звезды G 235-52" . ... Рис.1 Фотография объекта Рис.2 Фотография из второго . ... В 1999 и 2000 годах проводились наблюдения этого объекта на телескопе Цейсс-600 с целью подтверждения движения объекта. ... Используя данные, выводимые этой программой, мы измеряли расстояния между движущимся объектом и двумя ближайшими звездами. ... Величина собственного движения объекта 0.269'/год. ...

SUNWORLD - I. ZEEMAN - . 1964). ... J u - ( M = 0 ); -2 -1 -3 -2 -1 0 0 1 1 2 2 3 J l = 3, J u = 2 : = = 0 ­ M M begin J l end min( J l , J u ) : 3 = J J u r - ( -2 -1 0 0 1 1 M = -1 ); 2 2 3 J l = 3, J u = 2 M M begin = J l l -3 -2 -1 end = -1 : 2 = - ( J u - 1) J J u r - ( M = -1 ); 0 0 1 1 2 2 3 J l = 2, J u = 3 M M begin -3 -2 -1 -2 -1 = = J l l end = -2 = - ( J u - 1) , M begin M end , -. Unit ZEE, 1. ZEEMAN Unit ZEE - , , . ZEEMAN, INCLUDE- , 2. ... CalcGEff ZEEMAN INCLUDE : 1. ...

... Seminar archive . ... The structure of the X-ray sources in the hard spectral state of accreting black-hole binaries has been a subject of intense debate. The paradigm dominant for many years postulated that the accretion disc in the hard state is truncated at some radius >> the innermost stable orbit (ISCO) whereas the disc reaches the ISCO in the soft state. ... On the other hand, there have been numerous claims in recent years that the disc extends to the ISCO in the hard state. ...

Elsevier Ed itorial System(tm) for JASR 2006 Manuscript Draft Manuscript Number: Title: Determination of K, Ar, Cl, S, Si and Al flare abundances from RESIK soft X-ray spectra Article Type: Contributed Paper Section/Category: E2.4 - Solar Magnetic Field and Activities Keywords: solar physics; X-ray flares ; spectroscopy; abundances Corresponding Author: Dr. J. Sylwester , Corresponding Author's Institution: Space Research Center First Author: J ... All flares were observed early Fig. ...

... April 1992 The MD5 Message-Digest Algorithm Status of this Memo This memo provides information for the Internet community. ... combination): -sstring - digests string -t - runs time trial -x - runs test script filename - digests file (none) - digests standard input */ int main (argc, argv) int argc; Rivest [Page 17] RFC 1321 MD5 Message-Digest Algorithm April 1992 char *argv[]; { int i; if (argc 1) for (i = 1; i argc; i++) if (argv[i][0] == '-' argv[i][1] == 's') MDString (argv ...