... A laboratory approach to the interstellar sulfide problem. ... Optical constants: . ... The sulfides were synthesized from the native elements by the evacuated silica tube method with an annealing at 1273 K. The resulting sulfide powders were portioned, pressed to pellets, and melted in an arc furnace. The molten samples were quenched. For samples with x=0.0, 0.1, 0.25, 0.4, 0.5, 0.6, 0.75, 0.9, reflectance by polished surfaces was measured in the range from 2 to 500 microns. ...
D. Garofalo, D.A. Evans, R.M. Sambruna, MNRAS, 2010 D. Garofalo, D.A. Evans, R.M. Sambruna, MNRAS, 2010 D. Garofalo, D.A. Evans, R.M. Sambruna, MNRAS, 2010 A.Tchekhovskoy et al, ApJ, 699,1789, 2009 -: Magnetar: L j = 2 в 10 47 ( 1ms B R erg / s ) p 1015 G 10km 100 2 2 4 2 2 2 2 4 Black Hole: BH M BH k L j = 5 в 10 a 16 0 erg / s 10 G 3M 10 48 : BH with a < 0 M = 30 M (retrograde rotation) BH = 1012.5 G, a = -0.9 BH Cyg X-1 B ~ 100 . ...
... The package stsdas.graphics needs to be loaded (to run imdisp_pos for getting # the NDC's of the display image) # set imtype="fits" # print " " print " *** Start of impol FOC demo *** " print " [stecf.impol and stsdas.graphics need to be loaded] " print " " # # (First delete any model reflection nebulae left over from previous demos) # print " Deleting any old demo files " imdel reflneb1*.fits verify=yes # # An input (intensity) image is required. ... First delete any previous list files # ! ...
... Главная Астрономия Фотографии Рекорды Форум Гостевая книга . Азбука . ... Статьи по астрономии . Ваш путеводитель в мире астрономии . ... Статьи и рефераты по Астрономии / Астрономические Таблицы / Характеристики больших планет и их орбит . Характеристики внутренних планет . ... общая масса a . ... масса b (земля=1) . ... масса b (г) . ... сидерический круговой период . ... наклонение экватора к орбите . ... Характеристики внешних планет . ... Характеристики планетарных орбит . ...
Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...
T Ant [A/H] = -0.0. P var, nonlinear elements: Max = 2436120.756 T Ant + 5.897915d*E + 4.80d*10^{-8}E^2 [00027]. ... 00000]. ... Brightness variations with AG Ant the orbital period probably due to variations of circumstellar AG Ant extinction. ... R Ara Min II 6.2. ... The data in [00002] reveal RR Tel current V-band variations with a small amplitude and nearly RR Tel the same period [00000]. ... V0340 Tel The data from [00002] do not confirm the tabulated period V0340 Tel [00000]. ...
Zinovy Malkin: CPO Prediction: Accuracy Assessment and Impact on UT1 Intensive Results, IVS 2010 General Meeting Proceedings, p.261265 http://ivscc.gsfc.nasa.gov/publications/gm2010/malkin.pdf CPO Prediction: Accuracy Assessment and Impact on UT1 Intensive Results Zinovy Malkin Central Astronomical Observatory at Pulkovo of Russian Academy of Sciences e-mail: malkin@gao.spb.ru Abstract The UT1 Intensive results heavily depend on the celestial pole offset (CPO) model used during data processing. ...
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Microsymposium 34, MS058, 2001 ANOMALIES OF THE MOON'S THERMAL EMISSION IN THE IR SPECTRAL RANGE (10.5 - 12.5 micron). ... Sternberg State Astronomical Institute, Moscow, 119899, Russia, pugach@sai.msu.ru Summary: New satellite measurements of the lunar-surface radiation temperature were used to construct the spatial angular function of thermal radiation of the Moon in the infrared (10.5-12.5 micron) spectral range. ... These thermal anomalies are observed only in the limited range of phase angles. ...
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