... Suppose that a NS having a rotational magnetic   luminosity forms a binary system (with semi-major axis a ) with a normal star losing matter in the form of stellar wind (with a loss rate ). ... This means that while deriving the formula for a cavern in the general case, we must take into account the proximity of the normal star. ... It follows from the symmetry considerations that at the anterior point of the cavern (i.e. the point closest to the normal star), . ... If , the cavern is closed. ...

... 19 640 0.2482 0.00 17.148 ( ) 98.1 ( ) 248.54 () 6.387259 () 6.38725 () 6.38725 () 2306 1250 -220 -240А. . ... 300 - 400 - - 2005 FY9 - P = 308 a = 45.64 .., = 0.15, i = 29А 1500 , , , 2003 EL61 R = 51 .. a = 43.3 .., e = 0.19, i = 28А.2 - - , > 0.6 1960 з 1518 з 996 2500 з 1080 з 860 100 P = 3.9 , , 2003 EL61 S/2005 (136108) 1 () 49 500 0.050 (49.12 Б 0.03) 234А.8 Б 0А.3 S/2005 (136108) 2 39 300 0.0 (34.7 Б 0.1) 39АБ 6А S1 28% S1 3.3 mag S1 1% S1 1999 ., ... Л (New Horizons) 2006 ., - 2007 ., 2015 ...

... Информация Руководство и преподаватели Крутов Александр Федорович . ... Публикации . ... Krutov A.F. , Polezhaev R.G., Troitsky V.E. Describing radiation decay using the instant form of relativistic quantum mechanics // Theoretical and Mathematical Physics. 2015. ... Крутов А.Ф. , Полежаев Р.Г., Троицкий В.Е. Описание радиационных распадов в рамках мгновенной формы релятивистской квантовой механики // Теоретическая и математическая физика. ... 2014. ... Крутов А.Ф. 8 (846) 334-54-04 . ...

Work related with IAU C52: RIFA M.H. Soffel and W. Han Les Journees 2014, St. Petersburg, September 22 Main work - ecliptic in a relativistic framework - fully documented relativistic VLBI model Related work - the post-linear metric (PPN-metric for light rays) - models for bodies with higher spin-multipole moments Les Journees 2014, St. Petersburg, September 22 Ecliptic IAU 2006 Resolution B1: Recognizing 2. the need for a definition of the ecliptic for both astronomical and civil purposes .. ...

... Irreducible and full set of independent orthogonal dimensionless parameters in the `velocity normalised basis' Symbol M Ma Name Mach number Magnetic Mach ( Mach ­ AlfvИn) Strouhal Trieste numbers ( set ) Velocity-emission Formula / Definition Signifiance Temperature Governing MHD equations with dissipation and radiation v v c s S V vt x Magnetic ... DOI: 10.1016/j.asr.2005.03.084 ...

Lutsenko Olena L. (PhD, Psychology, Associate Professor) Filonenko Anna (Master, Psychology, Lecturer) School of Psychology V. N.Karazin Kharkiv National University COURSE DESCRIPTIONS ­ PSYCHOLOGY OF LEADERSHIP Title and N of module 1­ Leadership Theories Themes 1. ... Ethical leadership. ... Organizational Behavior and Human Decision Processes, 95 , 140-155. ... Socializing the newcomer: The mediating role of leader-member exchange.Organizational Behavior and Human Decision Processes, 119, 114-125. ...

... GALAXY: A galaxy is made up of billions or trillions of stars bound together by their own gravity. ... HELIUM (He): The second element in the periodic table, has 2 protons, 2 neutrons, and is a noble gas. ... Helium melts at -272.2 degrees Celsius, and boils at -268.934 degrees Celsius. ... HYDROGEN (H): The first element on the periodic table, is a gas, and has an atomic mass of 1.00794 amu. ... Hydrogen melts at -259.34 degrees Celsius, and freezes at -252.87 degrees Celsius. ...

. Spectrum-RG/eROSITA/Lobster                                                        Mission Definition Document            . 5 . Mission_Def_Doc_6.doc

Atm 2 ospheric time constant with MASS and FADE 0 A. Tokovinin CTIO, Chile Adaptive Optics time constant 0 = 0.314 r0/V0 = 0.057 6/5 [ Cn2(h) V5/3(h) dh MASS time constant: 0, MASS, Numerical simulation 1. Set turbulent layer strength (seeing) & sp. response Definition (1 rad phase difference between wavefronts at t= 0) ] 3/5 = 0.175 (2 DESI ) 3/5 ; 2 DESI = < [ IA(1ms)/ IA(3ms) ] >2 0, MASS, This is an approximation! ... The MASS method is approximate! ...

... Equinox of object coordinates BJ = 18.87 / bJ magnitude UMBJ = -0.69 / u - bJ colour BJMR = 0.22 / bJ - r colour NOBS = 1 / Number of 2dF observations available IS_ BEST = 'TRUE ' / TRUE if this file contains the best 2dF observa DATEBEST= '24/09/00' / Date of best 2dF observation (DD/MM/YY) ID_ BEST = 'QSO ' / ID from best 2dF observation QUALBEST= 11 / Data quality flag from best 2dF observation Z_ ...

... Submitted by Ben Kleschinsky on 11/02/2013 02:18:51 . Summer Solstice Super Moon 6/23/13 . Taken on the night of the Summer Solstice around midnight June 23, 2013. ... Camera: Nikon D5100 Lens: 70-300mm ED VR . Shutter-Speed: Unknown ISO: Unknown . POST PROCESSING: . ... Logon to post a follow-up comment or review comments from others . Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

A tree for site navigation will open here if you enable JavaScript in your browser. ... ABOUT ST-ECF . ... On this page we provide implementations of the the signal-to-noise ratio estimator DER_SNR following the definition set forth by the Spectral Container Working Group of ST-ECF, MAST and CADC. A detailed description and discussion of the algorithm can be found in the Issue #42 of the ST-ECF newsletter . ...

... Participant : The person whose name appears on the booking form. ... Participation Fee/ Optional Program Price . ... Passport and Visas . ... Travel insurance is highly recommended for all Participants while attending SpaceDTP-2016 and any related optional trips arranged by the Organizer. ... This booking condition states that the Participant must assume that he/she is not covered by the Organizer insurance policy including all liability insurance, for death, injury, damage or any other loss. ...