` . Minor Planets sorted by names .

B 3000 4000 5000 6000 7000 8000 ­0.001 ­0.001 ­0.000 0.000 0.001 0.001 ARP220 811300003 rec: 300 tm: 1:13:59 dps B1 B 3220 3240 3260 3280 3300 0.000 0.002 0.004 ARP220 811300003 rec: 300 tm: 1:13:59 dps B1

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. ...

... 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 ...

Ralph Sutherland RSAA, ANU, ANITA Cooling in the ISM Cooling in the ISM Example: Nearby RGs with Resolved Hosts M87 Sparkes et al 2004 astro-ph/0402204 Example: Active Galaxies: Cen A Example: Equilibrium Heating and Cooling : HII regions Example: Galactic ISM Example: Galactic ISM Example: z= 3.8 galaxy 4C41.7 4C41.17 Scharf et al 2003 Theoretical Approach: ISM thermal emission -12.0 II III I 0.0 -1.0 12.0 11.0 10.0 9.0 rec. eq. cool p r e IV V,VI -2.0 -3.0 -4.0 coll. cool eq. ...

... Глава 2 . ... Ссылка из Главы 4 ). ... 0015+0501 . ... 0105+0501 . ... 19000 .008 . ... 3000 .010 . ... 450 .008 . ... 4000 .008 . ... 0444+0501 . ... 3000 .0502 . ... 3000 .011 . ... 0.64 . ... 3000 .014 . ... 12000 .008 . ... 1429+0501 . ... 1436+0501 . ... 3000 .034 . ... 500 .008 . ... 3000 .1613 . ... 1646+0501 . ... 1000 .008 . ... 3000 .0040 . ...

... 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 ...

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 ] ...

... 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 .. ...

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

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 . ...

... 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 . ...

filter wavelength Calculated V1 Calculated V2 Abs Wave ; ------ ---------- ------------- ------------- -------- S I r 1 3 -1.5298 -639.0000 -662.0000 6561.5000 3 -1.2287 -420.0000 - 599.0000 6561.8000 3 -1.0279 -274.0000 -557.0000 6562.0000 3 -0.8272 -128.0000 -515.0000 6562.2000 3 -0.6264 18.0000 -473.0000 6562.4000 3 - 0.4298 161.0000 -432.0000 6562.6000 3 - 0.3294 234.0000 -411.0000 6562.7000 3 - 0.2291 307.0000 -390.0000 6562.8000 3 - ...

... Удель. элек. новое старое началь-я сила, при H=20 А/см, сопр-е, обозначение макс-я А/см Тл Ом*мм2/м 1411 Э31 250 5500 0.44 1.52 0.52 1511 Э41 300 6000 0.36 1.49 0.6 1512 Э42 400 7000 0.32 1.49 0.6 1561 Э45 600 10000 0.2 7.7*10^-4~ 0.55 1562 Э46 600 7000 --- 8.8*10^-4~ 0.55 1572 Э48 600 7000 --- 1.3~2 0.55 3411 Э310 500 16000 0.2 1.81 0.5 3412 Э320 800 33000 0.12 1.73 --- ----------------------------------------------------------------------- ~ При H=8 мА/см и толщине листа 0.35 мм ~2 При H=10 А/м 2....

... edetect_chain (edetect_chain-3.0) [xmmsas_20080701_1801-8.0.0] . ... 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'' . ...

... 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 ...

... Каталог MEADE по сериям . ... Рефракторы апохроматы 6000 ED Triplet APO . ... Оптическая труба апохромат 6000 серии 130mm ED TRIPLET APO (f/7) с фокусировщиком Крейфорда . ... MEADE представляет рефрактор 130 ED Triplet APO из модельного ряда 6000 ED. Этот инструмент является своего рода произведением искусства, т.к. обладает выдающимися оптическими характеристиками и представляет собой классический апохромат премиум-класса с объективом-триплетом из стекла со сверхнизким показателем дисперсии. ...

... 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. ...