` . Minor Planets sorted by names .

Number of Pre and Post anneal hotpixels 80000 70000 60000 # Hot Pixels # Hot Pixels 50000 40000 30000 20000 10000 0 1995 4000 3500 3000 # Hot Pixels # Hot Pixels 2500 2000 1500 1000 500 0 1995 2000 2005 2010 Decimal Year 2015 2020 0 1995 2000 2005 2010 Decimal Year 2015 2020 2000 2005 2010 Decimal Year 2015 ...

Impact ­ Produced Exosphere of Europa A.A. Berezhnoy Sternberg Astronomical Institute, Moscow, Russia Equilibrium chemical composition of the impact-induced cloud 0.5 0.45 0.4 0.35 0.3 0.25 0.2 0.15 0.1 3000 3500 4000 T, K 4500 OH H2 5000 O 5500 H H2O Q 0.0045 0.004 0.0035 0.003 0.0025 0.002 0.0015 0.001 0.0005 0 2000 Na NaO H NaO 3000 T, K 4000 5000 1.E-01 2000 Q 1.E-02 1.E-03 1.E-04 T, K 2500 CO 3000 ... Previous detection of cometary impacts on Europa is very tentative. ...

... T A B * * Extinction table for LPO. ... SET .Z.LABEL = Extinction * 3000 3.7150 3100 1.5961 3200 0.9908 3300 0.6967 3400 0.5934 3500 0.5146 3600 0.4554 3700 0.4061 3800 0.3633 3900 0.3260 ... 9200 0.0099 9300 0.0095 9400 0.0091 9500 0.0087 9600 0.0083 9700 0.0080 9800 0.0077 9900 0.0074 10000 0.0071 10100 0.0068 10200 0.0065 10300 0.0063 10400 0.0060 10500 0.0058 10600 0.0056 10700 0.0054 10800 0.0052 10900 0.0050 11000 0.0048 ...

... 4 3000 3500 4000 4500 5000 5500 6000 6500 7000 7500 8000 8500 9000 Tarusa 19.01.2012 - p. 9 Time dependent at 15 Day 1.8з10 14 15 day H, CA time dep endent f (er g /s/cm2/H z ) 0. ... 6 3000 3500 4000 4500 5000 5500 6000 6500 7000 7500 8000 8500 9000 Tarusa 19.01.2012 - p. 10 Steady state, time dependent at 15 Day 1.8з10 14 15 day H, CA time dep endent steady state f (er g /s/cm2/H z ) 0. ... 2 3000 3500 4000 4500 5000 5500 6000 6500 7000 7500 8000 8500 9000 Tarusa 19.01.2012 - p. 21 ...

Добро пожаловать, Гость . ... На форуме начался конкурс - Астрофотография месяца: АПРЕЛЬ! ... Астрофотография (Модераторы: Павел Бахтинов , Ivan Mhitarov ) ? Logitech QC 4000 и 5000 . ... 0 Пользователей и 1 Гость просматривают эту тему. ... Рейтинг: +19/-3 . Ответ #40 : 08.01.2006 [00:19:13] ? ... Записан . ... Рейтинг: +126/-2 . ... Гость . ... Рейтинг: +369/-27 . ...

B?rbel Koribalski (ATNF) + HIPASS and ZOA teams . Velocities are color coded in bins of 1000 km/s: . dark blue . ... light blue . cross . 1000 . green . ... HVCs? ... All the new galaxies, most of which are at |b| All the new galaxies are marked in blue, HI clouds in green and HVCs in orange. (plot by Malte Marquarding, aips++). bkoribal @ atnf.csiro.au ...

КОЭФ-ТЫ ПОГЛОЩ. ... ИОНОМ ВОДОРОДА К.У.АЛЛЕН АСТРОФИЗИЧЕСКИЕ ВЕЛИЧИНЫ "МИР",М.,1977Г.,С.98 СТОЛБЦОВ 7 СТРОК 6 #LG_KAPPA_H_MINUS &(A)\THETA 0.5 0.6 0.8 1.0 1.2 1.6 2.0 ---------------------------------------------------------- 3000. ... 3.91 4.15 4.60 4.97 5.31 5.93 6.46 10000. 3.95 4.17 4.63 5.03 5.33 5.94 6.52 ---------------------------------------------------------- КОЭФ-ТЫ РАСЧИТАНЫ НА ОДИН НЕЙТРАЛЬНЫЙ АТОМ ВОДОРОДА И НА ЕДИНИЦУ ЭЛЕКТРОННОГО ДАВЛЕНИЯ LG A(H-) [ A(H-) В 1.0Е-30 СМ^4/ДИН ] ...

... Е К К Н ЙОМ ОМНН НЛП H (t ) q2 (t ) = q1 (t ) k2 a(t ) tз q2 > q ?К?К Д ? Е К t 1 К Н ЙОМ ОМНН ОЛП ? ... Е К К Н ЙОМ ОМНН ЛП ?К?К Д ? ... Е К К Н ЙОМ ОМНН ЛП 6000 5000 l(l+1)C / 2 [ЕK2] 4000 3000 2000 1000 0 WMAP Abelian Higgs strings Semilocal strings Textures l 10 1 10 multipole moment: l 2 10 3 ?К?К Д ? ... Е К К Н ЙОМ ОМНН ПМ Л П НО V () = 4 exp(-/0 )И Н О M Pl К И N e 60 -5 П / PS 5 З 10 r = PT /PS < 0.2 К И И ns = 0.94 ? ... Е К К Н ЙОМ ОМНН ПН Л П НП И НММ V () = m2 2 /2 НМ К К ?К?К Д ? ...

HIinARP220 3000 4000 5000 6000 7000 8000 Velocity [km/s] ­0.10 ­0.08 ­0.06 ­0.04 ­0.02 0.00 0.02 Intensity [Jy]

... Allow the common mo de and differential mo de signal to b e a linear of combination of CARM and DARM. Fit results: common = 4.7 CARM + 0.8 DARM diff = 1.4 CARM + 5.1 DARM Common Mo de Graph 50 40 30 10 20 5 10 0 -10 -20 -30 0 1000 2000 3000 4000 5000 0 -5 -10 -15 -20 0 1000 2000 3000 4000 5000 20 15 Differential Mo de Graph Time in minutes , displacement in microns Official calibration common diff = = 6.5 CARM 2.7 CARM + + 2.7 DARM 6.5 ...

True Color Image Gallery: Galactic SNR | ... Left: raw image, binned by, 4 x 4, pixel(s) . Right: gaussian smoothed version of above (sigma = 2 pixel [in binned image]) Click left mouse button on hyperlink below to download file . All the FITS files in this page as TAR file . ... Images . ... PS File . FITS files . unsmoothed (raw/exposure) . smoothed . raw image (counts) . exposure map . ... Back to G39.2-0.3 Index . Chandra Supernova Remnant Catalog . ...

... Rv(j) [mkm] / Xv(j) / a/b(j) / ksi(j)/V(j)/Vtotal j= 3 1.0000 0.0000*i 0.110 mkm, 1.386, 4.24910, 0.2421, 0.3330 j= 2 1.5000 0.0000*i 0.139 mkm, 1.747, 2.52137, 0.4320, 0.6660 j= 1 3.0000 0.0000*i 0.159 mkm, 2.000, 2.00000, 0.5774, 1.0000 .. ... Rv(j) [mkm] / Xv(j) / a/b(j) / ksi(j)/V(j)/Vtotal j= 3 1.0000 0.0000*i 0.110 mkm, 1.386, 3.04315, 1.0588, 0.3330 j= 2 1.5000 0.0000*i 0.139 mkm, 1.747, 2.30830, 1.1095, 0.6660 j= 1 3.0000 0.0000*i 0.159 mkm, 2.000, 2.00000, 1.1547, 1.0000 .. ...

... For example, the previous examples are periodic. Example Dual beam calibration observation of a strong-point source with the GBT: Example Dual beam calibration observation of a strong-point source with the GBT: 0 -1 -2 Tb -3 -4 0 1000 2000 3000 t 4000 5000 6000 Example 1/f spectrum Shor t section of the data away from the strong source Time stream Power spectral density -1.75 -1.76 -1.77 -1.78 -1.79 240 260 280 300 t 320 340 360 15 5 5 15 25 0.0 0.2 0.4 Frequency 0.6 Power ...

... edetect_chain (edetect_chain-2.16.2) [xmmsas_20060628_1801-7.0.0] . ... edetect_chain imagesets=''M1IMAGE_1000.FIT M1IMAGE_2000.FIT M1IMAGE_3000.FIT M1IMAGE_4000.FIT M1IMAGE_5000.FIT'' \ eventsets=M1EVLI.FIT \ attitudeset=atthk.dat \ pimin=''200 500 2000 4500 7500'' \ pimax=''500 2000 4500 7500 12000'' \ ecf=''1.8035 1.9872 0.75557 0.26502 0.028794'' . ...

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... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... 1 Comparison between white dwarf and solar synthetic emergent fluxes per unit area at the emitting photosphere. ... Since there are several ways planets can survive the giant phase of the host star, we examine the habitability and detection of planets orbiting white dwarfs. As a white dwarf cools from 6000 K to 4000 K, a planet orbiting at 0.01 AU would remain in the Continuous Habitable Zone (CHZ) for 8 Gyr. ...

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

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