... There are two stars in the binary system: a donor star on the right and a black hole on the left (an infinitely small point in the center of a complex figure). ... The wind is ejected as a hollow cone; it has a funnel (the funnel opening angle in the figure) and thick walls (wall opening angle in the figure). The observer looks at the whole system and the supercritical disk from the right, and sees everything up to the wind photosphere (the red color in the figure). ...

... SWXCS J000315-5255.2 . ... SWXCS J000324-5253.8 . ... SWXCS J002437-5803.9 . ... SWXCS J005500-3852.4 . ... SWXCS J011432-4828.6 . ... SWXCS J021705-5014.2 . ... SWXCS J021747-5003.4 . ... SWXCS J023924-2505.1 . ... SWXCS J035259-0043.7 . ... SWXCS J044144-1115.6 . ... SWXCS J062155-6228.6 . ... SWXCS J082113+3200.1 . ... SWXCS J084749+1331.7 . ... SWXCS J085524+1102.0 . ... SWXCS J090946+4157.2 . ... SWXCS J092729+3010.8 . ... SWXCS J092650+3013.8 . ... SWXCS J092719+3013.7 . ...

. Приложение к лекции для студентов . Верходанов О.В. Рис.12. Пример работы алгоритма чистки. На верхнем рисунке приводится модельное изображение, на среднем - грязная карта, на нижнем - изображение, восстановленное с помощью CLEAN. Рисунок воспроизведен из работы Стиэра и др. (1984). vo @ sao.ru ( Oleg Verkhodanov ) .

... Поверхностная фотометрия галактик . ... В Приложении мы приводим несколько таблиц, которые могут быть полезны при интерпретации результатов поверхностной фотометрии. Характеристики широкополосной системы . ... Показатели цвета нормальных галактик . ... 0.55 . ... Публикации с ключевыми словами: Фотометрическая система - слабые галактики - Скопление галактик - фотометрия . Публикации со словами: Фотометрическая система - слабые галактики - Скопление галактик - фотометрия . ...

... В Приложении мы приводим несколько таблиц, которые могут быть полезны при интерпретации результатов поверхностной фотометрии. Характеристики широкополосной системы . ... в системе Джонсона-Моргана/Казинса (по [ 130 , 282 ]) . и в системе Бесселя и Бретта [ 283 ] (по [ 143 ]) . ... 0.55 . ... одиночной вспышки звездообразования, в системе . Джонсона-Моргана/Казинса и в системе Бесселя и Бретта . ... в системе Джонсона-Моргана (по [ 285 ]) . ...

... Flux Sign Expo . ... Flux, mCrab . ... 0.80 PHA . ... IGR J16318-4848 . ... The map above is movable . ... Flux map Error map Significance Exposure . Flux and error maps are in mCrab units. All maps are convolved with instrumental point spread function (PSF) which is Gaussian ( =5'). Exposure maps are in ksec. INTEGRAL/IBIS 9-year Galactic Hard X-Ray Survey* , A , Volume 545, id.A27 { NASA ADS | ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ...

... We chose the stellar model (log Teff = 4.33668, log g 0 = 4.07842) calculated with OPAL opacities. ... We considered Kurucz's (1994) model atmospheres ) 14 Daszynska and Cugier 0.80 0.80 0.80 =0.95 0.75 l=0 0.75 0.70 l=1 m=0 0.75 0.70 l=1 m=-1 F /10-9 + Offset [erg cm-2 s-1 nm-1] 0.70 0.65 0.65 0.65 0.60 0.60 0.60 0.55 0.55 0.55 0.50 0.50 0.50 0.45 0.45 0.45 0.40 =0.0 0.40 0.40 0.35 0.35 0.35 a) 0.30 455.15 455.20 455.25 b) 455.35 0.30 455.15 455.20 455.25 c) 455.35 ...

... Погружения поверхностей в $R^3$ и основная проблема их классификации с точностью до регулярной гомотопии и кобордизма. ... A. Определение групп $Imm^o(n,1)$ и $Imm^{so}(n,1)$. ... Imm^{so}(0;1)$ степень отображения. ... B. Устойчивые отображения. Нормальная локальная форма устойчивых отображений. ... Пример вычисления алгебраического числа особенностей $I$-cтруктуры коразмерности 1 при регулярной гомотопии двух устойчивых погружений и гомотопии двух устойчивых отображений. ...

... 000, 000ґ000 (2010) Printed 16 June 2010 A (MN L TEX style file v2.2) Molecular outflows in the Perseus molecular cloud ґ supporting online only material Spectra of outflow detections are in Figs. ... Figure 1 ґ continued c 2010 RAS, MNRAS 000, 000ґ000 Molecular outflows in the Perseus molecular cloud ґ supplement 3 Figure 1 ґ continued c 2010 RAS, MNRAS 000, 000ґ000 4 E. I. Curtis et al. ... Spectra of sources with no outflow detections in IC348. c 2010 RAS, MNRAS 000, 000ґ000 8 E. I. Curtis et al....

Приложение 2. ... figure . subplot(2,1,1); . plot(t,y) . zoom xon . yfft=abs(fft(y)); . ... plot(freal, abs(h)) . plot(freal, abs(h).*abs(h)) . ... title ('а') . ... soutfft=abs(fft(sout1)); . ... flen=length(fhis); . ... plot(fhis(1:flen),sumyfft1(1:flen)) . ... plot(fhis(1:flen),sumsoutfft1(1:flen)) . ... plot(fhis(1:flen),sigrechis(1:flen)) . ... plot(freal, abs(h).*abs(h),'r',... fhis(2:flen), sigrechis(2:flen).*sigrechis(2:flen)) %,... % fhis(2:flen), sumsigrec2(2:flen)) . ...

... If the Earth is round, the Sun must be north of the equator in northern summer, and south of the equator in northern winter. ... From the Earth's perspective, the Sun is spiraling from north to south and back again along the ecliptic (see figure 7 ). ... The round Earth, at the summer solstice. ... If the rotation axis of the Earth is tilted with respect to its orbit, the equator bobs back and forth, causing the Sun to be north for half the year, and south for the other half (see figure 9 ). ...

... This model shows unstable l = 0, 1 and 2 modes of oscillations. ... We considered Kurucz's (1994) model atmospheres 14 Daszynska and Cugier 455.15 455.20 455.25 455.30 455.35 0.30 0.35 0.40 0.45 0.50 0.55 0.60 0.65 0.70 0.75 0.80 l=0 a) f=0.0 f=0.95 F l /10 ґ9 + Offset [erg cm ґ2 s ґ1 nm ґ1 ] l [nm] 455.15 455.20 455.25 455.30 455.35 0.30 0.35 0.40 0.45 0.50 0.55 0.60 0.65 0.70 0.75 0.80 l=1 m=0 b) l [nm] 455.15 455.20 455.25 455.30 455.35 0.30 0.35 0.40 0.45 ...

... Article text . ... Article should be formatted according to the present rules, using the styles containing in the attached file example.doc . ... For example, article name should be typed in string Here Is the Paper Title , using style "title paper", etc. ... Title part of article Paper Title (style Title Paper . ... It is necessary to use style text paper for the body of article. ... In the text of article there should be links to every Figure and Table: Fig. 1 and Tab. 1 accordingly. ...

... HOME . ... MICROSCOPES . ... SURGICAL MICROSCOPES . ... Home Products Microscopes Laboroscopes Phase Contrast/Brightfield/Darkfield Condenser (C-PHM) N.A. 0.80. PHASE CONTRAST / BRIGHTFIELD / DARKFIELD CONDENSER (C-PHM) N.A. 0.80. ... It incorporates phase annulus rings for 10X/20X, 40X and 100X objectives as well as Brightfield and Darkfield positions.The phase annuli are easily centerable with two knurled alignment knobs. ...

Full-Text Search . ... arXiv.org . astro-ph . ... SAI VO . Search sort results by Date Relevance . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . Normalized to: Figures, 1. 1 article(s) in total . 4 co-authors, from 1 to 2 common article(s). Median position in authors list is 5,0 . Co-author(s): . ... request, available upon. ... Astronet | SAI MSU . ...

обзор! astro-ph/0207130 . ... Author: Bertil Dorch . Comments: Invited review, IAU coll. ... В обзоре рассматривается трехмерное моделирование магнитных трубок на Солнце. ... Comments: 55 pages, 35 figures -- low resolution figures to allow upload to astro-ph High-resolution version at http://www-sgk.harvard.edu:1080/~sylvain/preprints/ . ... Comments: 6 pages, 4 figures, Astron Nachr (accepted; proceedings of "1st Potsdam Thinkshop on Sunspots and Starspots", Potsdam, Germany, May 2002) . ...

XMM-Newton CCF Release Note XMM-CCF-REL-174 pn telescope e ective area modi cation M. Kirsch June 9, 2004 1 CCF components Name of CCF VALDATE List of Blocks changed CAL VERSION XSCS ag XRT3 XAREAEF 0009 2000-01-13T00:00:00 ONAXISXAREAEF 3.169 NO 2 Changes XMM EPIC-pn observations with very high statistic show residuals at the Silicon edge around 1.8 keV and gold edge around 2.2 keV (see Figure 1). The gold edge feature can be explained by not perfect calibration of the telescope e ective area. ...

and 42 % 27-11-1999 Andr\'as Holl % 2.31: 02-05-2001 % % Konkoly Observatory, Budapest, Hungary % Use the following documentstyle definition : % \documentstyle[twoside, ibvs2, epsf]{article} % or % \documentstyle[twoside]{article} % \input ibvs2.sty % \input epsf.sty % epsf is only needed for figures % IBVS.STY screen message \ typeout {} \ typeout {IBVS.STY Ver. 2.31 - 02-05-2001 } \ typeout {Information Bulletin on Variable Stars - Konkoly Observatory} \ ...

Computer Ephemeris for 2015 from DE200/LE200. Ecliptical coordinates of the Sun. 98356743 -23.392 5.353 -0.226 5.043 15 Th 37.5 2942953.05 0.08 -0.11 0.98362696 -23.254 5.372 -0.252 5.022 16 Fr 38.5 2953100.50 0.19 0.00 0.98369109 -23.116 5.390 -0.237 5.000 17 Sa 39.5 2963207.75 0.27 0.09 0.98375953 -22.978 5.406 -0.181 4.983 18 Su 40.5 2973314.74 0.33 0.15 0.98383199 -22.841 5.421 -0.091 4.979 19 Mo 41.5 2983421.39 0.35 0.18 0.98390819 -22.703 5.435 0.018 4.995 20 Tu 42.5 2993527.59 ...

... Several analysis strategies for computation of systematic part in the radio source velocities can be used: a) estimate source position and velocities from global solution, then fit spherical harmonics to the velocities (Gwinn et al. 1997); b) compute the coefficients of spherical harmonics as global parameters (MacMillan 2005; Titov 2008); c) compute velocities from position time series, then fit spherical harmonics to the velocities. ... Time series statistics is shown in Table 1. ...