... Armagh Observatory 2001 July */ #declare Shining_Dwarf_Core = sphere{ 0,0,0 , 0.99 hollow on interior{ media{ absorption rgb 0.0 , 0.0 , 0.0 scattering { 5 rgb 1.0 , 1.0 , 1.0 eccentricity + 0.1 } density { spherical color_map{ [0.00 rgb 0,0,0 ] [ 0.05 rgb 0.1 , 0.1 , 0.5 ] [ 0.2 rgb 0.2 , 0.2 , 0.6 ] [ 0.5 rgb ...

... The current SNR catalogue is at http://www.mrao.cam.ac.uk/surveys/snrs/ Jump to l =360œ . 1st quadrant: G0.0 + 0.0 G0.3 + 0.0 G0.9 + 0.1 G1.0 - 0.1 G1.4 - 0.1 G1.9 + 0.3 G3.7 - 0.2 G3.8 + 0.3 G4.2 -3.5 G4.5 +6.8 G4.8 +6.2 G5.2 -2.6 G5.4 -1.2 G5.5 + 0.3 G5.9 +3.1 G6.1 + 0.5 G6.1 +1.2 G6.4 - 0.1 G6.4 +4.0 G6.5 - 0.4 G7.0 - 0.1 G7.2 + 0.2 G7.7 -3.7 G8.3 - 0.0 G8.7 -5.0 G8.7 - 0.1 G8.9 + 0.4 G9.7 - 0.0 G9.8 +0.6 G9.9 -0.8 G10.5 - 0.0 G11.0 - 0.0 G11.1 -1.0 G11.1 -0.7 G11.1 + ...

Òåìà : Õâîñòàòûå ãîñòüè: îòêðûòèÿ - ïåðåîòêðûòèÿ êîìåò äî 2012 ãîäà âêëþ÷èòåëüíî .. Ïîêàçàòü ñîîáùåíèå îòäåëüíî . 02.11.2012, 14:13 . ... P/2012 K4 (Larson) = P/2005 N3 (Larson) = 261P/Larson .. P/2012 K4 (Larson) = P/2005 N3 (Larson) = 261P/Larson, MPEC 2012-K54 , CBET 3123 . Ýëåìåíòû îðáèòû êîìåòû P/2012 K4 (Larson) = P/2005 N3 (Larson) = 261P/Larson: . Epoch 2012 Sept. ... T 2012 Sept. ... Ýôåìåðèäû êîìåòû P/2012 K4 (Larson) = P/2005 N3 (Larson) = 261P/Larson: . ...

... with known photometry from the catalog by Blaha and Humphreys (1989) OB-ass. l b r Vr dvr nr mul dml mub dmb nm Nt SGR OB5 0.0 - 1.2 2.4 -15.0 19.0 2 0.1 1.7 0.1 2.2 3 31 SGR OB1 7.6 - 0.8 1.3 -10.0 12.1 37 -1.6 1.2 -1.3 1.0 29 66 SGR OB7 10.7 -1.6 1.4 -6.1 17.1 3 -0.0 0.3 -3.3 0.1 2 4 SGR OB4 12.1 - 1.0 1.9 3.5 10.8 9 - 0.7 1.4 - 0.8 2.5 3 15 SER OB1 16.7 0.1 1.5 -5.0 20.0 17 - 0.7 ...

Change in Brightness Kepler 4b 0.0 % - 0.1 %0.12 - 0.2 % 0.14 0.16 0.18 0.02 0.04 0.06 0.08 Transit Light Curves Set 1 Transit Tracks p. 3 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-7b 0.0 % -1.0% -2.0% 0.2 0.4 0.6 0.8 1.2 1.4 1.6 1.8 2.2 2.4 2.6 2 4 6 8 10 12 14 16 Time (in days ) 18 20 22 24 26 Change in Brightness HAT-P-11b 0.0 % -0.5% -1.0% ...

COS Instrument Handbook for Cycle 24 . ... Cosmic Origins SpectrographInstrument Handbook for Cycle 24 > Chapter 10: Bright-Object Protection > 10.4 Source V Magnitude Limits . ... 6.9 . ... KM III (Eta Ser) . ... KM III (Alpha Boo) . ... KM III (Gamma Aql) . ... KM III (HD 146051) . ... KM III (Alpha Cet) . ... KM III (HD 123023) . ... KM III (Beta Gru) . ...

from __future__ import division from visual import * scene = display(range=(3.0,3.0,3.0),width=1300,height=800,forward=( 0.2 ,-0.3,-1.0)) water = box( pos =(0,- 0.1 , 0.0 ), length=10, width=3, height= 0.1 , color =( 0.1 , 0.2 ,1.0)) alength = 2.0 theta = 0.1 pos1 = vector (0,0,0.6) barge1 = box( pos = pos1, length = 2, width = 0.5, height = 0.1 , color =(0.6,0.4, 0.2 )) x1 = arrow( pos = pos1+ vector (0, 0.1 ,0), ...

default { finish { ambient 0.4 } } camera { up 0, 1, 0 right 1, 0, 0 location -1,3,-16 look_at 0,0,0 angle 40 } light_source { 10,10,-10 color rgb 1,1,1 } #declare deskwood_streaks = pigment { bozo color _map { [ 0.0 color rgb 0.25, 0.2 ,0.1 ] [ 0.4 color rgb 0.5, 0.4 , 0.2 ] [0.5 color rgb 0.68, 0.6 ,0.45 ] [ 1.0 color ...

... Ñïðàâî÷íèê ïî áèïîëÿðíûì òðàíçèñòîðàì . Òðàíçèñòîðû 2ÒÑ641 - ÊÒ680 . ... 40-150/100 . ... 0.2 . ... 40-120/150 . 100-300/150 . ... 200 . ... 0.4(150/15) . ... 20-200/150 . ... 40-200/200 . 150- /200 . ... 100-300/ . ... 25-100/500 . ... 100 . ... 40-150/150 . 80-250/150 . ... 200-450/2 . ... 0.5(500/50) . ... 50-160/200 . ...

Ìàðñ â 2014 ãîäó: . ... Ñêëîíåíèå ÐäÑ ÐäÇ mag Ýëîíã.Ñîçâ. ------------------------------------------------------------------------- 1 ÿíâ 12h45m29.67s -02 31' 41.9 1.6660 1.3649 0.8 88.8 Vir 6 ÿíâ 12h53m35.28s -03 19' 10.1 1.6660 1.3149 0.8 91.8 Vir 11 ÿíâ 13h01m18.88s -04 03' 46.2 1.6657 1.2648 0.7 94.8 Vir 16 ÿíâ 13h08m38.25s -04 45' 16.6 1.6652 1.2148 0.6 97.9 Vir 21 ÿíâ 13h15m30.52s -05 23' 26.3 1.6645 1.1650 0.5 101.2 ...

DIMM . ... 100 000 , 2007 ­ 2009 . ... S 0.2). ... 1 3 ) , D DIMM. s DIMM s= D r0 5/3 = 5 D 2 · l2,t , Kl,t (1 4 ) 1.0 S a 0.9 0.8 0.7 LE MTF SE MTF S a 0.6 0.5 0.4 0.3 0.2 0 1 2 3 4 5 6 5/3 7 8 9 10 s = (D/r0) . ... Smin > 0.45, Smin < 0.45, - DIMM, 7 - 8 . ... Smin > 0.45 ( ) Smin < 0.45 , . ... Smin > 0.3 7 l / 0.8 0.6 S o t 1.0 0.4 0.2 Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep 2008 2009 . ... 8 MASS/DIMM 2007 2009 , , , , . ...

... 4 0.08567 3.83484 8447.35 yes - ¢¢¡¡ ¢¢¡¡ ¢ ¢ ¢¡ ¡ ¢¡ ¡ 0.3 G302.486-00.030 c2h 0.3 G302.486-00.030 hcn 0.3 G302.486-00.030 hnc 0.2 0.2 0.2 Average Intensity (Jy/ beam ) Average Intensity (Jy/ beam ) 0.1 0.1 Average Intensity (Jy/ beam ) 0.1 0.0 0.0 0.0 0.1 0.1 0.1 0.2120 100 80 60 Velocity (km/s) 40 20 0 0.2120 100 80 60 ...

... The problems of complexity in coagulation: specification 1. ... Numerical experiments Task 1: Activation threshold Final clot density VS activation : model reduction Factor V is activated 7 6 7 6 No factor V activation Fibrin 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Fibrin 5 5 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Activation Activation y= Ae ( Bx 1 ) y = Ax Final clot density VS activation : the experiment Fibrin clot density (a.u.) 1.0 0.8 0.6 0.4 0.2 ...

... INTERVAL TD C/S (mb) C/S ALMA-ATA 891022 3600 070000-080000 00 1101.80 681.0 1101.80 0.6 ALMA-ATA 891022 3600 080000-090000 00 1107.48 680.8 1105.89 1.0 ALMA-ATA 891022 3600 090000-100000 00 1112.46 680.6 1109.26 1.3 ALMA-ATA 891022 3600 100000-110000 00 1109.05 680.7 1106.66 1.0 ALMA-ATA 891022 3600 110000-120000 00 1110.33 680.5 1106.34 1.0 ALMA-ATA 891022 ...

Rfmonitor data:100401 .5*(maxAllowable exposure) 1.6 1.4 1.2 1.0 0.8 0.6 0.4 0.2 5 10 15 Hour of day Ast 20 Rfmonitor data:100701 .5*(maxAllowable exposure) 1.6 1.4 1.2 1.0 0.8 0.6 0.4 0.2 5 10 15 Hour of day Ast 20 Rfmonitor data:100801 .5*(maxAllowable exposure) 1.0 0.5 0.0 -0.5 -1.0 -1.5 5 10 15 Hour of day Ast 20 Rfmonitor data:101001 .5*(maxAllowable exposure) 4.10 4.05 4.00 3.95 3.90 5 10 15 Hour of day Ast 20

... where zmax is maximum of GJ (z ) ~ at z zmax the solution satisfied both conditions exists E|| = 0 and (B · )E|| = 0 29 10 28 5 gradual rapid Bsc / Bdi p 10 27 0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1.0 0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1.0 Bsc / Bdip 8. only photon absorption in magnetic field no photon splitting, photon scattering Yu.E. Lyubarskii A A 261 544 (1992) Bdip = 1.0 · 1012G, P = 3 · 106 years, = Lpc from [18] is ... ApJ, V.615, p.908 (2004) [22] A.T.Deller et al...

... Abstract: We present Monte Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk and a two-phase clumpy dust distribution. ... As a general result, clumpy models are less opaque than the corresponding homogeneous models. ... 0.00 0.15 0.50 0.1 0.5 1.0 2.0 5.0 10.0 0.25 X . ... We have also produced several homogeneous models, to compare to the clumpy models. ... Homogeneous and clumpy models with the same tauV have the same dust mass. ...

... Ïîïîâ Àíäðåé Àëåêñååâè÷ . ... Ìîñêâà . ... Ðîññèÿ . ... 8.0 . ... Âëàñîâ Àíäðåé Äìèòðèåâè÷ . ...

... DZ *= (+1.2 + 1.7) óãë. ñåê. ...  òå÷åíèå 40 ìèí. òåëåñêîï ñîïðîâîæäàë îáúåêò òîëüêî ïðîãðàììíûì âåäåíèåì (îáëà÷íîñòü) è ïðè ïîÿâëåíèè îáúåêòà íàáëþäàòåëü ââåë ïîïðàâêè êîððåêöèè (+ 0.1 è - 0.3 ) óãë. ñåê., íî äàæå è ýòè ïîïðàâêè áûëè óñòðàíåíû ñëåäóþùåé êîððåêöèåé ( ñì. ðèñ. 3 è òàáë. 2 è 3 ). ... Îòñþäà ìîæíî ñäåëàòü âûâîä, ÷òî ïðè íàáëþäåíèÿõ ñ ÏÇÑ-êàìåðîé ÏÔ ÁÒÀ íàêîïëåííàÿ îøèáêà ïðîãðàììíîãî âåäåíèÿ ÁÒÀ íå ïðåâûøàåò çíà÷åíèé (0.1 - 0.2) óãë. ñåê., òî-åñòü ˜ 0.1 ðàçìåðà èçîáðàæåíèé (âñå îöåíêè...

... 673 Table Mountain Observatory, W rightwood. ... 703 Catalina Sky Survey. ... H 19.0 seconds of 0.0 0.5+ 0.8- 1.6+ 1.0+ 0.21.0- 0.11.2+ 1.00.2+ 0.0 0.4- 0.5+ 0.6- 0.41.6+ 0.1 + 0.6- 0.10.4- 0.50.5- 0.10.8- 1.91.4- 1.3- 15.89003 +0.55234657 -0.27174286 G 0.15 U9 arc 090818 151 0.1 + 0.4+ 090819 H26 0.0 0.4090818 B04 0.5+ 0.0 090819 695 1.1- 0.6+ 090818 151 0.1 + 0.6+ 090819 673 0.3- 0.0 090818 B04 0.6+ 0.0 090819 673 0.1 + 0.1090818 B04 0.5+ 0.0 ...