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Ïîêàçàíû äîêóìåíòû, ñîäåðæàùèå ôðàãìåíòû òåêñòà èç äîêóìåíòà
http://www.mrao.cam.ac.uk/projects/surveys/snrs/snrs.data.html.
http://www.mrao.cam.ac.uk/projects/surveys/snrs/snrs.data.html.
1. Galactic SNRs: FRAMESET list
... 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 + ...
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Ññûëêè http://www.mrao.cam.ac.uk/projects/surveys/snrs-2006/snrs.f_list.html -- 18.0 Êá -- 10.04.2016
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2358) - www.mrao.cam.ac.uk/ )
2. Îáùàÿ Àñòðîíîìè÷åñêàÿ Êîíôåðåíöèÿ - Ïîêàçàòü ñîîáùåíèå îòäåëüíî - Õâîñòàòûå
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: . ...
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Ññûëêè http://www.starlab.ru/showpost.php?p=467705&postcount=294 -- 21.1 Êá -- 12.04.2016
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3. http://star.arm.ac.uk/~csj/movies/povray/stars.inc
... 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 ...
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Ññûëêè http://star.arm.ac.uk/~csj/movies/povray/stars.inc -- 6.6 Êá -- 29.03.2002
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>976) - star.arm.ac.uk/ )
4. http://www.mso.anu.edu.au/pfrancis/simulations/barges_light.py
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), ...
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Ññûëêè http://www.mso.anu.edu.au/pfrancis/simulations/barges_light.py -- 5.7 Êá -- 15.04.2014
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>310) - www.mso.anu.edu.au/ )
5. http://hea-www.harvard.edu/~pgreen/AGASCupdate/numspoilers2.sort
... 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 ...
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Ññûëêè http://hea-www.harvard.edu/~pgreen/AGASCupdate/numspoilers2.sort -- 3.0 Êá -- 27.06.2000
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>1177) - hea-www.harvard.edu/ )
6. The supernova remnants (SNRs) radio maps, optical and X-ray images (l=0-360deg)
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 . ...
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Ññûëêè http://www.sao.ru/cats/~satr/SNR/snr_dir.html -- 29.8 Êá -- 17.01.2002
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>787) - www.sao.ru/ )
7. http://www.atnf.csiro.au/research/hypercompact/talks/Titmarsh.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 ...
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Ññûëêè http://www.atnf.csiro.au/research/hypercompact/talks/Titmarsh.pdf -- 909.3 Êá -- 08.09.2010
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>10079) - www.atnf.csiro.au/ )
8. http://lnfm1.sai.msu.ru/~anna/kinem-OB-ass.txt
... 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 ...
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Ññûëêè http://lnfm1.sai.msu.ru/~anna/kinem-OB-ass.txt -- 9.2 Êá -- 07.03.2003
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9. http://www.astrosociety.org/edu/publications/tnl/76/8lightcurves.pdf
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% ...
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Ññûëêè http://www.astrosociety.org/edu/publications/tnl/76/8lightcurves.pdf -- 703.1 Êá -- 02.10.2012
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>137) - www.astrosociety.org/ )
10. Model PSFs
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 . ...
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Ññûëêè http://www.stsci.edu/instruments/wfpc2/Wfpc2_hand2/ch5_psf6.html -- 117.4 Êá -- 29.08.2000
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>7388) - www.stsci.edu/ )
11. Ñàòóðí 2014
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 ...
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Ññûëêè http://edu.zelenogorsk.ru/astron/planets/satu14.htm -- 7.0 Êá -- 27.02.2014
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>405) - edu.zelenogorsk.ru/ )
12. http://curl.sai.msu.ru/mass/download/doc/shtrel_control.pdf
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 , , , , . ...
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Ññûëêè http://curl.sai.msu.ru/mass/download/doc/shtrel_control.pdf -- 196.0 Êá -- 03.01.2010
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>31) - curl.sai.msu.ru/ )
13. http://hea.iki.rssi.ru/Z-90/arc/21/Oh.key/angles_single_bounce.pdf
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
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Ññûëêè http://hea.iki.rssi.ru/Z-90/arc/21/Oh.key/angles_single_bounce.pdf -- 28.9 Êá -- 27.12.2004
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>519) - hea.iki.rssi.ru/ )
14. Galactic SNRs: Summary Data
... Sgr A East 0.3 +0.0 17 43 05 -28 37 15x8 S 22 0.6 0.9 +0.1 17 44 12 -28 08 8 C 18? varies 1.0 -0.1 17 46 20 -28 25 8 S 15 0.6? ... 1.9 +0.3 17 45 37 -27 09 1.2 S 0.6 0.7 3.7 -0.2 17 52 20 -25 50 11x14 S 2.3 0.65 3.8 +0.3 17 49 50 -25 27 18 S? 4? ... 7.7 -3.7 18 14 20 -24 05 22 S 11 0.32 1814-24 8.7 -5.0 18 21 05 -23 50 26 S 4.4 0.3 8.7 -0.1 18 02 35 -21 25 45 S? 80 0.5 (W30) 9.8 +0.6 18 02 10 -20 14 12 S 3.9 0.5 10.0 -0.3 18 05 40 -20 26 8? ... 0.5 345.7 -0.2 17 03 50 -40 49 6 S 0.6? ...
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Ññûëêè http://www.naic.edu/~pulsar/catalogs/snrs.data.html -- 22.6 Êá -- 05.08.1999
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>1360) - www.naic.edu/ )
15. http://www.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf
... 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 ...
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Ññûëêè http://www.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf -- 183.8 Êá -- 24.02.2010
[ Òåêñò ] Ññûëêè http://mavr.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf -- 183.8 Êá -- 01.10.2009
Ïîõîæèå äîêóìåíòû
[ Òåêñò ] Ññûëêè http://mavr.sao.ru/hq/katya/NDG/DVD/Talks/Kurbatov.pdf -- 183.8 Êá -- 01.10.2009
Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>647) - mavr.sao.ru/ )
16. Change history
... 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 . ...
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Ññûëêè http://xmm.vilspa.esa.es/sas/7.1.0/doc/epreject/node2.html -- 5.5 Êá -- 15.11.2007
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>2690) - xmm.vilspa.esa.es/ )
17. http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C044/O/SH221089.AAB
... 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 ...
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Ññûëêè http://www.wdcb.ru/stp/data/cosmic.ray/G%20L%20E/C044/O/SH221089.AAB -- 14.0 Êá -- 20.06.2005
Ïîõîæèå äîêóìåíòû
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>1225) - www.wdcb.ru/ )
18. Optical constant database - Level: data
. 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.
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Ññûëêè http://www.astro.spbu.ru/JPDOC/PAPERS/HENNING.95/mgfeo.html -- 3.0 Êá -- 19.11.2010
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Ïîõîæèå äîêóìåíòû
Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>169) - www.astro.spbu.ru/ )
19. ÓÒÂÅÐÆÄÀÞ
... 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...
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Ññûëêè http://mavr.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://www.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://jet.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
Ïîõîæèå äîêóìåíòû
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://www.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
[ Ñîõðàíåííàÿ êîïèÿ ] Ññûëêè http://jet.sao.ru/hq/sekbta/Navedenie/spravka.htm -- 300.9 Êá -- 20.08.2013
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Åùå â ðàçäåëå:
(Ïîêàçàòü âñå ðåçóëüòàòû (>635) - jet.sao.ru/ )
20. http://www.mccme.ru/albio/slides/panteleev.pdf
... 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 ...
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Ññûëêè http://www.mccme.ru/albio/slides/panteleev.pdf -- 2897.4 Êá -- 09.10.2008
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