... 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 + ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>1986) - www.mrao.cam.ac.uk/ )

• Galactic SNRs: Detailed Listings

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: . ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>3325) - www.starlab.ru/ )

• Îáùàÿ Àñòðîíîìè÷åñêàÿ Êîíôåðåíöèÿ - Ïîêàçàòü ñîîáùåíèå îòäåëüíî - P/2013 PE67 /
• P/2013 PE67 / A/2013 PE67 (Catalina) / VG3AFFD object .. [Àðõèâ] - Îáùàÿ
• Àñòåðîèä 2014 EP12 (Apollo, ? = 28 ì) 14 ìàðòà 2014 ãîäà â 0.007381632 a.e.

... 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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>778) - star.arm.ac.uk/ )

• http://star.arm.ac.uk/~meb/weather/md_dec14
• http://star.arm.ac.uk/~meb/weather/md_feb15
• http://star.arm.ac.uk/~meb/weather/md_jan15

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), ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>280) - www.mso.anu.edu.au/ )

• http://www.mso.anu.edu.au/pfrancis/simulations/barges.py
• http://www.mso.anu.edu.au/pfrancis/simulations/XRB.py
• http://www.mso.anu.edu.au/pfrancis/simulations/pulsar.py

... 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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>1029) - hea-www.harvard.edu/ )

• http://hea-www.harvard.edu/~fine/POV/src/fakewood.pov
• http://hea-www.harvard.edu/~fine/POV/src/tp_spare.pov
• http://hea-www.harvard.edu/~fine/POV/src/dual_towel_rod.pov

... 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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>266) - lnfm1.sai.msu.ru/ )

• http://lnfm1.sai.msu.ru/~olympiad/1997/files/prob1997prac.pdf
• http://lnfm1.sai.msu.ru/grav/russian/life/chteniya/sagi2007/kuzin.pdf
• http://lnfm1.sai.msu.ru/grav/russian/life/chteniya/sagit2008/Tatevyan.pdf

... 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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>9479) - www.atnf.csiro.au/ )

• INTRODUCTION

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% ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>41) - www.astrosociety.org/ )

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 . ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>651) - www.sao.ru/ )

• Ñïðàâî÷íèê ïî áèïîëÿðíûì òðàíçèñòîðàì
• SNRs Spectra Request Form
• Ñïðàâî÷íèê ïî ïîëóïðîâîäíèêîâûì äèîäàì

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 . ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>6269) - www.stsci.edu/ )

• COS Instrument Handbook
• Red Leaks in UV Filters

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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>535) - edu.zelenogorsk.ru/ )

• Ìåðêóðèé 2015
• Ýôåìåðèäà Ñàòóðíà 2004ã.
• Ìåðêóðèé 2009

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

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>416) - hea.iki.rssi.ru/ )

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 , , , , . ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>30) - curl.sai.msu.ru/ )

• http://curl.sai.msu.ru/mass/download/doc/dimm_spec.pdf

... 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 . ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>2437) - xmm.vilspa.esa.es/ )

... 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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>1171) - www.wdcb.ru/ )

• http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C042/O/SH290989.AAT
• http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C043/O/SH191089.AAB

. 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.

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>157) - www.astro.spbu.ru/ )

• Database of Optical Constants -- Level: group of materials

... 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...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>567) - jet.sao.ru/ )

• Ðàáîòà ñ ïðîãðàììîé bta_list.

... 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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>82) - www.mccme.ru/ )

• Algebra-1 (Fall 2015)

... 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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>29) - www.winer.org/ )

• http://www.winer.org/Downloads/MPEC2008-Y29.pdf
• http://www.winer.org/Downloads/MPEC2009-B39.pdf
• http://www.winer.org/Downloads/MPEC2010-A38.pdf

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 ...

Åùå â ðàçäåëå: (Ïîêàçàòü âñå ðåçóëüòàòû (>5859) - www.arcetri.astro.it/ )

• Traffic Analysis for ge-0/0/3 -- arcrt1