... 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 16 (êîððåêöèè îðáèòû) .. Ïîêàçàòü ñîîáùåíèå îòäåëüíî . ... Ñîîáùåíèé: 19,465 . Re: Õâîñòàòûå ãîñòüè (êîððåêöèè îðáèòû) .. ... Ýëåìåíòû îðáèòû êîìåòû C/2011 W3 (Lovejoy): . ... Îòïðàâèòü ëè÷íîå ñîîáùåíèå äëÿ Silvester . Íàéòè åùå ñîîáùåíèÿ îò Silvester . ...

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), ...

... 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 ...

... 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 ...

New SNRs (280-360deg) (Duncan+ 1997) . SNR mag. fields maps (Milne 1987) . ... G000.9+0.1 . ... G016.7+0.1 . ... G033.6+0.1 . ... G059.5+0.1 . ... G304.6+0.1 . ... G318.2+0.1 . ... G323.5+0.1 . ... G332.4+0.1 . ... G335.2+0.1 . ... G338.5+0.1 . ... G348.5+0.1 . ... G351.2+0.1 . ... G354.1+0.1 . ...

... MAGin-MAGspoiler #Spoiled Input Stars -5.7 1 -5.2 1 -5.0 1 -4.6 1 -4.4 1 -4.2 2 -4.1 1 -4.0 2 -3.9 2 -3.8 1 -3.7 2 -3.6 3 -3.4 1 -3.3 1 -3.2 2 -3.1 2 -3.0 2 -2.9 1 -2 ... .7 2 -2.6 3 -2.5 1 -2.4 5 -2.3 5 -2.2 5 -2.1 3 -2.0 4 -1.9 2 -1.8 4 -1.7 11 -1.6 4 -1.5 7 -1.4 11 -1.3 8 -1.2 15 -1.1 8 -1.0 8 - 0.9 18 - 0.8 12 - 0.7 19 - 0.6 15 - 0.5 14 - 0.4 17 - 0.3 22 - 0.2 12 - 0.1 18 0.0 13 0.1 19 0.2 23 0.3 11 0.4 15 ...

... 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% ...

Ñàòóðí â 2014 ãîäó: . ... Ïðîòèâîñòîÿíèå - 11 ìàÿ â Âåñàõ, óãëîâîé äèàìåòð 18.7" . ... Ñêëîíåíèå ÐäÑ ÐäÇ mag Ýëîíã.Ñîçâ. -------------------------------------------------------------------- 1 ÿíâ 15h13m17.61s -15 41' 29.9 9.881 10.482 0.6 50.2 Lib 6 ÿíâ 15h15m03.84s -15 47' 45.6 9.882 10.416 0.6 54.8 Lib 11 ÿíâ 15h16m43.25s -15 53' 27.2 9.883 10.346 0.6 59.5 Lib 16 ÿíâ 15h18m15.36s -15 58' 33.7 9.884 10.272 0.6 64.2 Lib 21 ÿíâ 15h19m39.66s -16 03' 04.2 9.885 10.196 ...

Considerable effort has gone into the modeling of the HST point spread function (PSF), both in order to measure the optical aberrations in support of the WFPC2, COSTAR, and advanced scientific instruments, and to provide PSFs for image deconvolution in the aberrated telescope. ... As a consequence of the under-sampling in the WFPC2, the limiting magnitude attainable in the background limit varies by about 0.5 magnitude, depending on the position of the source within the CCD pixel. ... 0.9 . ...

... 6 5.5 5 4.5 5.5 6 6.5 7 7.5 8 8.5 9 -1.33 -1.34 -1.35 -1.36 -1.37 -1.38 4.5 5 5.5 6 6.5 7 7.5 8 L - [Z] 0.4 0.38 0.36 0.34 0.32 0.3 0.28 4.5 5 5.5 6 6.5 7 7.5 8 L - [Fe] 0.85 0.8 5.5 6 6.5 7 7.5 8 8.5 9 0.95 0.9 M-L 1.05 1 M - M/L 13/14 M = 106.5 Msol 0.3 [Fe/H] 0.2 OB = 2 km/s 0.3 M = 106.5 Msol OB = 8 km/s 0.3 M = 107.5 Msol OB = 8 km/s 0.3 M = 108.5 Msol OB = 8 km/s [Fe/H] 0.2 0.2 [Fe/H] 0.2 [Fe/H] 0.1 0.1 0.1 ...

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 , , , , . ...

. Mg x Fe 1-x O from Henning et al. (1995) . Use our codes to transform the standard data file to another form. Back to paper page . Last modified: 25/09/98, V.I.

Surface Scattering Angle Surface Point Source, Isotropic Emitter into Sphere 1 0.9 0.8 0.7 0.6 P["] 0.5 0.4 0.3 0.2 0.1 0 0 !/4 !/2 Scattering " 3!/4 ! MC: local line center resonant MC: local HG scattering, g=0.0 Analytic HG, g=-1/3

... 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 ...

Recycled stellar ejecta as fuel for star formation Marijke Seger s, Rob Crain, Joop Schaye (Leiden Obser vator y) 0.5 Fraction contributed by recycling 0.4 35% 19% SFR Stellar mass AGB stars SN Type Ia Massive stars 0.3 Cosmological SPH simulation: Evolution and Assembly of GaLaxies and their Environments (EAGLE) At z = 0, 35% of the cosmic SFR density and 19% of the cosmic stellar mass density is ...

... 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...

... 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 ...

... offset correction values now read from file . ... offset columns, selected bad pixels & columns, . ... offset correction thresholds now per pixel . ... sigma threshold for offset correction added; . mask rows 1-15 set to bad . ... detailed task description added . ... task description updated . ... description of soft flare screening added . ... new parameters: -set, -withoffsetmap . new algorithm: energy correction calculated . directly from offset maps . ...