Peremennye Zvezdy ( Variable Stars ) 33 , No. ... We present our discovery a new variable star USNO-A2.0 1350-17086180 from observations at the Astrotel-Caucasus Observatory. ... The numbers of observations on each of the observing nights are presented in Table 1; the observations are attached to the html version of this paper. ... Numbers of observations . ... No. observations . ... 0.001 . ... 0.000 . ... 0.003 . ... 0.004 . ... 0.002 . ... 0.005 . ...

F(6 cm) Other Name ct/s erg cm -2 s -1 µJy FX/FR mJy # r B R Class z Catalogs WGAJ0011.2- 3620 0.002 1.73E - 14 0.003 -12.73 96 0.12 21.3 FSRQ 2.324 WGAJ0012.5- 1629 0.097 1.28E - 12 0.29 -10.53 50 0.62 17.7 FSRQ 0.151 1 WGAJ0015.5+ 3052 0.019 2.82E - 13 0.083 -11.37 89 0.62 16.3 17.2 FSRQ 1.619 0.023 3.16E - 13 0.095 WGAJ0029.0+ 0509 0.006 6.33E - 14 0.014 -12.71 377 0.00 19.3 18.1 FSRQ 1.633 WGAJ0032.5- 2849 ...

... Cal steps adopted for freq 4946.00 1.31 1.54 GTP : 3.560 6.034 0.008 0.004 SDO : -0.018 0.000 0.002 0.002 !205/03:17:40.8 (UT) status: idle 205/03:17:40.8 75.04 84.95 0.00 0.00 0.00 GTP : 3.560 6.034 0.008 0.004 SDO : -0.006 0.000 0.000 0.000 set fine atten to 5466 GTP : 3.561 6.034 0.008 0.004 SDO : -0.020 0.000 - ...

... Name Designation ff ffi J (ffi J ) H (ffi H ) K (ffi K ) J \Gamma K H \Gamma K Nights a AS01­0 FS02 00 55 09.9 00 43 13 10.716 ( 0.005 ) 10.507 ( 0.010 ) 10.470 (0.003) 0.25 0.04 6,6,6 AS02­0 SAO054271 00 55 58.6 39 10 09 8.775 (0.006) 8.771 ( 0.012 ) 8.770 ( 0.009 ) 0.01 0.00 5,6,6 AS03­0 FS03 01 04 21.6 04 13 39 12.606 ( 0.011 ) 12.729 ( 0.008 ) 12.827 ( 0.013 ) ­0.22 ­0.10 6,6,6 AS04­0 FS04 01 54 37.6 00 43 01 10.555 (0.004) 10.301 ( ...

... The designations are given for each object along with J2000.0 coordinates, followed by three columns for each filter, containing the magnitude, the first standard deviation or scatter among data points, and the number of measurements N. The values reported for the magnitudes are weighted averages, using 1/(sigma)^2 weighting, where the sigmas are the internal photometric errors of individual measurements." ... 0.005 . ... 0.008 . ... 0.006 . ... 0.007 . ...

J1347+122 3.630.10 4 3.640.10 4 3.650.10 4 3.660.10 4 3.670.10 4 3.680.10 4 3.690.10 4 Heliocentric Velocity (Km/s) 0.000 0.002 0.004 0.006 0.008 0.010 Fractional Absorption 36300 36500 36700 36900 Heliocentric Velocity (km/sec) 0.002 0.0 0.004 0.006 0.008 Fractional Absorption 0.01 J1347+122

... Глава 2 . ... Ссылка из Главы 4 ). ... 4.3 . ...

... RJMCMC Similar to Richardson Green 1997 Knowledge of the PSF makes things easier Insensitive to e.g. posterior for ten sources with = 3: Number of Components 9 10 11 12 0.141 0.222 0.220 0.157 0.022 0.029 0.027 0.021 Mean SD 7 0.029 0.018 8 0.058 0.019 13 0.082 0.014 Simulated Data Source region (2 SD) is about 28% of the area and contains about 41% of the observations Positions (-2, 0), (0, 1), (1.5, 0) with intensities ... Approximate the number of sources (2 in this case) 2. ...

... Инерциальные характеристики Амальтеи . ... Обобщенные моменты инерции . Полностью нормализованные стоксовы коэфиициенты разложения внешнего гравитационного поля Амальтеи (9 степени и порядка) . ... Для вычисления выбрана гармоническая модель топографии 18 порядка и степени. ... Приводятся Стоксовы коэффициенты до 9 порядка и степени. ... Виды Амальтеи с шести взаимно перпендикулярных направлений, вычисленные на основе гармонического разложения топографии (используется модель 18 порядка и степени). ...

Kepler-11 . KIC 6541920 . KOI-157 . ... открыта в 2011 году . 0.091+0.001 . 0.006+0.004 . 0.161+0.002 . 10.3039+0.001 . ... 0.107+0.001 . ... 0.256+0.002 . ... 0.155+0.001 . ... 0.278+0.002 . ... 0.004+0.007 . ... 0.195+0.002 . ... 0.373+0.002 . ... 0.25+0.002 . ... 0.466+0.004 . ... 0.297+0.002 . 118.3807+0.001 . ... 1 Уникальная система Kepler-11 - шесть транзитных планет в плотной упаковке . 2 Все 6 планет в системе Kepler-11 имеют низкую плотность ...

... Data It is now clear that fuzzballs are actually galaxies. ... Using the automatic telescope, we measured the redshifts and brightnesses of a large number of fuzzballs in all regions of the sky. ... Correlation between brightness and redshift Redshifts and Brightnesses 0.005 0.004 0.003 0.002 0.001 0 -0.001 0 -0.002 -0.003 -0.004 -0.005 Redshift of Fuzzball 500 1000 1500 2000 Brightness of Fuzzball The brightnesses and redshifts of all the fuzzballs measured are shown in this graph. ...

... Nearly all the sources have com­ plete data at 2.3, 3.9, 7.7 and 11.2 GHz; 40 sources have 21.7 GHz flux densities. ... Fluxes of the sources in the NCP region Name, S 0.325 # t S 1.4 # t S 2.3 # t S 3.9 # t S 7.7 # t S 11.2 # t S 21.7 # t Sp. index NVSS Jy, WENSS Jy, NVSS Jy Jy Jy Jy Jy # 0.325/11.2 J000943+772440 2.059 0.082 0.628 0.021 0.447 0.04 0.267 0.017 0.161 0.007 0.14 0.016 -- -- 0.76 J001236+854313 1.605 0.064 0.691 0.023 0.539 0.048 0.246 0.018 0.148 ...

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. ...

... 60 спутников в порядке удаления от планеты) . ... Спутник . ... 128 000 . 0.3 . ... 129 000 . ... 181 400 . ... 671 100 . ... 0.000 . ... 1 070 400 . ... 1 882 700 . ... 7 507 000 . ... 11 165 000 . ... 11 461 000 . ... 11 717 000 . ... 11 741 000 . ... 12 555 000 . ... S/2003 J20 Carpo . ... 17 056 000 . ... S/2003 J3 . ... S/2003 J12 . ... S/2001 J10 Euporie . ... 19 394 000 . ... 20 216 000 . ... S/2003 J18 . ... 20 700 000 . ... S/2003 J6 Helike . ... 20 979 100 . ... 21 000 000 . ... Юпитер | ...

Spectrum Teff_1 +/- lg g1 +/- nHe_1 +/- vsini1 +/- q_1 +/- dv_1 +/- chi^2 bd10op.sp2 17.760 0.002 2.664 0.004 0.989 0.000 33.47 0.19 1.00 0.00 136.0 0.0 9.31E+00 bd10op.sp2 17.760 0.000 2.664 0.000 0.997 0.000 33.47 0.00 1.00 0.00 136.0 0.0 9.06E+00 bd10op.sp2 17.998 0.002 2.736 0.004 0.997 0.000 33.47 0.00 1.00 0.00 136.0 0.0 9.00E+00

... New period of the third body in the system of the eclipsing HgMn binary star AR Aur was derived based on new photoelectric and CCD observations. 1 Intro duction AR Aur (HD 34364, HR 1728) is a double­lined spectroscopic well­detached eclipsing binary with orbital period of 4d 13. ... Circles -- minima times computed by our method, squares -- minima times adopted from literature. minima determinations published new periods of the third body and new physical characteristics of the system. ...

... Зор? до 2.5 зоряно? величини . ... Паралакс . ... F2 III . ... Ведмедиц? ... Великого Пса ( Мурз?м ) . ... Великого Пса ( Сир?ус ) . ... Великого Пса ( Адара ) . ... Астроном?чна одиниця (а.о.): . ... Тобто р?чний паралакс св?тила це кут, п?д яким з цього св?тила видно середн?й рад?ус земно? орб?ти. ... В?н означа?, на ск?льки зоряних величин зоря в короткохвильов?й д?лянц? спектра яскрав?ша (слабша), н?ж у довгохвильов?й. Прийнято, що B V = 0 для з?р спектрального класу A0 головно? посл?довност?. ...

... 01.04.2009 . ... 0.000 . ... 0.281 . ... 2.0806 . ... 0.002 . ... 0.004 . ... 0.341 . ... 0.001 . ... 0.332 . ...

... 000, 1­17; (2005) Printed 28 March 2006 A (MN L TEX style file v2.2) The star formation history of early-type galaxies as a function of mass and environment M.S. Clemens1 , A. Bressan 1 2 3 4 1,2 INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio, 5, 35122 Padova, Italy. ... We calculate the Lick indices for the entire sample and correct for aperture effects and velocity dispersion in a model independent way. ... 2005). ... The mean velocity dispersion is higher in denser environments...

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