... The current SNR catalogue is at http://www.mrao.cam.ac.uk/surveys/snrs/ Jump to l =360њ . 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 + ...

Тема : Хвостатые гостьи: открытия - переоткрытия комет до 2012 года включительно .. Показать сообщение отдельно . 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 . Элементы орбиты кометы P/2012 K4 (Larson) = P/2005 N3 (Larson) = 261P/Larson: . Epoch 2012 Sept. ... T 2012 Sept. ... Эфемериды кометы P/2012 K4 (Larson) = P/2005 N3 (Larson) = 261P/Larson: . ...

... 6161: FOC Aperture location appears to be off by 1 arcsec. ... FOC team supported Phase II proposal development . ... The Bright Object Camera: Part 2 нн ND Filters SPACE TELESCOPESCIENCE INSTITUTE TIPS Meeting 22 Feb 1996 Mark Voit Summary of FOC Activities for the period 18 January 1996 -- 21 February 1996 SPACE TELESCOPESCIENCE INSTITUTE TIPS Meeting 22 Feb 1996 Mark Voit Summary of FOC Activities for the period 18 January 1996 -- 21 February ...

... SiO Line Ratios log([J=1-0 v=3]/[J=1-0 v=2]) log([J=1-0 v=2]/[J=1-0 v=1]) 1.6 1.2 0.8 0.4 0 log([J=1-0 v=3]/[J=1-0 v=1]) corr: 0.59 A 1 corr: 0.40 C 0 -1 -0.4 -0.8 -1.2 -0.6 0.5 0 -2 -0.4 -0.2 0 0.2 0.4 0.6 0.8 -3 -0.6 -0.4 -0.2 log(F25/F12) 0 0.2 0.4 0.6 0.8 corr: 0.35 B -0.5 -1 -1.5 -2 l Detections in both lines s Upper limits r Lower limits 0.8 -2.5 -0.6 -0.4 -0.2 0 0.2 0.4 0.6 log(F25/F12) log(F25/F12) vs. ...

... Справочник по биполярным транзисторам . Транзисторы 2ТС641 - КТ680 . ... 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 . ...

declare chrome = texture { pigment { color rgbf 0.5 0.5 0.5 0 } finish { diffuse 0.1 specular 0.5 reflection 0.7 roughness 0.005 metallic } } #declare tp_holder= union { cylinder { 0,0,0 0,0, 0.2 1.3 } torus { 1.3 0.1 rotate 90*x translate 0.1 *z } cylinder { 0,0,0 0,0, 0.3 1.15 } torus { 1.15 0.1 rotate 90*x translate 0.2 *z } cylinder { 0,0,0 0,0, ...

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), ...

Сатурн в 2005 году: . ... Максимальный блеск: -0,38m - 14 января 2005 . ... 1 Янв 07h47m09.14s +21њ08' 33.7 9.058 8.102 - 0.3 165.7 Gem 11 Янв 07h43m45.20s +21 18' 11.2 9.059 8.077 - 0.4 176.7 Gem 21 Янв 07h40m17.27s +21 27' 42.0 9.060 8.084 - 0.3 172.2 Gem 31 Янв 07h36m57.55s +21 36' 36.0 9.061 8.122 - 0.3 161.3 Gem 10 Фев 07h33m57.22s +21 44' 29.4 9.062 8.191 - 0.2 150.4 Gem 20 Фев 07h31m26.61s +21 51' 03.7 9.063 8.286 - 0.2 139.8 ...

SN 2006gi @ NOT on 19 Sep 2006 0.4 0.2 0.0 Lg(F) -0.2 -0.4 -0.6 -0.8 SN 1990I @ max -1.0 4000 5000 SN 1984L @ +8I 6000 7000 Wavelength(Angstrom) 8000 9000

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

N.N. Kolesnikov, A.A. Kolchin, D.L. Alov, Yu.N. Ivanov, A.A. Chernov, M. Schiber, H. Hermon, R.B. James, M.S. Goorsky, H. Yoon, J. Toney, B. Brunett, T.E. Schlesinger. Growth and characterization of p-type Cd 1- x Zn x Te( x = 0.2, 0.3, 0.4). Abstract: . Single crystals of p-type semi-insulating Cd 1- x Zn x Te (CZT) with x = 0.2, 0.3 and 0.4 were grown using the high-pressure vertical Bridgman method. ...

... 0.5 . ... 10o . ...

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% ...

... OH, = 18 cm Nancay Radio Telescope, OH 18-cm line observations , since 1969 F, Jy 6 4 2 0 0 -1 -2 0 -1 -2 0 -2 -4 -6 30 40 50 1612 MHz I HU Pup August 5, 2009 1665 MHz 4 2 0 0.5 0.0 - 0.5 -1.0 -1.5 1.0 0.5 0.0 - 0.5 4 3 2 1 0 -1 1667 MHz I I 1.0 0.5 0.0 0.5 0.0 22-meter telescope, Pushchino Radio Astronomy Observatory H2O F, Jy 1.0 0.5 0.0 0.4 0.2 0.0 -0.2 -0.4 0.4 0.2 0.0 -0.2 -0.4 -0.6 0.6 0.4 0.2 0.0 -0.2 -0.4 -70 -60 -50 -40 -30 -20 -10 0 Mira-type star R Leo. ...

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 , , , , . ...

... material . ... Tool (1910) Phys.Rev. 31, 1 . ... e 1,2 [fig] . ... Clemens, Jaumann (1963) Z.Physik 173, 135. cryst. ... Yolken, Kruger (1965) J.Opt.Soc.Am. ... Lenham, Treherne (1966) J.Opt.Soc.Am. ... cryst. ... refl. [fig] . ... Blodgett, Spicer (1967) Phys.Rev. 158, 514 . ... abs. [fig] . ... 1979) Phys.Rev. B19, 3850. cryst. ... Lynch, Hunter (1991) in Palik E. (ed) Handbook of Optical Constants of Solids, II. ... Lynch, Hunter (1998) in Palik E. (ed) Handbook of Optical Constants of Solids,...

Wind Dir Wind Speed Total Vis Present State Of Rainfall Sunshine 30cm 100cm Maximum Minimum Grass Cloud Weather Ground Min 1 2 2015 1009.2 -0.1 -0.5 290 5 1 6 2 16 0.30 5.7 5.0 7.1 5.5 -1.8 -7.3 2 2 2015 1010.6 0.0 -0.2 250 5 7 6 2 15 0.05 4.4 4.6 7.1 5.5 -2.0 -6.2 3 2 2015 1013.2 -1.5 -1.5 250 5 9 2 45 11 0.00 0.4 4.6 7.0 2.1 -5.3 -8.3 4 2 2015 1027.0 -3.2 -3.5 250 5 1 7 2 4 0.00 5.1 4.1 7.0 ...

HD 108863 . HIP 61020 . ... Расстояние от Солнца . ... Масса ( солнечных масс ) . ... Радиус (солнечных радиусов) . ... 0.2+0.03 . ... полуось , а.е. m sin i , . масс Юпитера . ... Расстояние в перицентре - 1.33 а.е. Расстояние в апоцентре - 1.47 а.е. Радиус эффективной земной орбиты (показана зеленым цветом) - 4.1 а.е. Новости о системе: . ...

Sternberg Astronomical Institute Lomonosov Moscow State University Time Series Prediction Leonid Zotov Fulbright Scholar 2008-2009 San Juan, Puerto Rico, 8 May 2009 FROM THE BEGINNING OF THE HISTORY PEOPLE TRIED TO PREDICT FUTURE "We remember only past events, not future ones." ...

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 ...