... 0.109 0.163 0.094 0.115 0.189 0.067 0.160 0.003 0.004 0.076 0.082 0.102 0.073 0.053 0.106 0.078 0.043 NGC1336 E 5.467 4.850 1.489 3.033 4.700 1.643 4.899 0.097 0.237 4.172 2.703 2.325 1.510 0.815 -4.815 -1.344 1.920 +- . 0.146 0.210 0.112 0.158 0.233 0.095 0.210 0.005 0.006 0.100 0.115 0.133 0.099 0.081 0.167 0.102 0.064 NGC1339 E 5.934 6.148 1.885 3.780 7.688 1.520 5.630 0.168 0.321 4.985 3.038 2.724 1.960 0.926 -6.111 -1.912 1.886 +- . ...

... QSO . ... 2006.07 . 2007.03 . ... 2008.04 . ... 0.079 0.018 . ... 0.187 0.022 . ... 0.198 0.018 . ... 0.146 0.016 . 0.135 0.016 . ... 0.149 0.022 . ... 0.254 0.022 . ... 0.263 0.018 . ... 0.271 0.016 . ... 0.223 0.022 . 0.178 0.022 . ... 0.535 0.022 . ... 0.702 0.022 . ... 0.269 0.018 . ... 0.180 0.016 . ... 0.221 0.018 . ... 0.389 0.018 . 0.428 0.018 . ... 0.142 0.016 . ... 0.114 0.016 . ... 0.129 0.016 . ... 0.498 0.022 . 0.523 0.016 . ... 1.065 0.022 . ... 1.097 0.018 . ...

Peremennye Zvezdy ( Variable Stars ) 35 , No. ... A. V. Khruslov . ... According to these data, the stars are double-mode RR Lyrae variables, pulsating in the first-overtone and fundamental modes. ... The author of the present paper, with his co-authors, earlier discovered 112 double-mode RR Lyrae variable stars, pulsating in the fundamental and first-overtone radial modes ( Khruslov 2007, 2010, 2011, 2012a,b, 2014, 2015; Khruslov et al. ... Information on the studied stars is presented in Tables 1-3. ...

... эЗЮЫ^ 1. ъвдТТЮТЬЫТ ЬЗЮТЬЫШ ,,ЮЫЮТТ,Аi вдлкЬЫЭг , ,ЬлкЫ дТЫг 1986 -2005 ,,,,. хгЯТЬк ?ЫвЮг сТЬЫкЬАТ шТЫг ЬЗЮТЬЫШ дгкЫ,г- дЮвкЫ- ввкгfl(,,г, ЯТвfl^, ТЬИ) вкгflЬЫfl ЬгЭ ЬЫfl, ,, 1986 1987 1988 1989 1990 1992 1993 1998 1999 2000 2001 2004 2005 10 09 10 12 12 03 04 09 08 09 12 03 03 17- 1987 30- 1988 05-1989 05-1990 16- 1991 07-1992 10-1993 02- 1999 19- ... ЩФщ. 1987. < 204. ы. 57-64. фЫвТЮТ, э.ш. ФвкгЯТкЫ~ТвЭЫТ ЬЗЮТЬЫfl ,,ЮЫЮТТ,Аi вдлкЬЫЭг, ?дЫкТ , шлЮЭг,Т Ь 26-ШЯг,гЯ ТйЭкгТ // рС,. ...

... Printed in U.S.A. The Hipparcos and Tycho Photometric System Passbands MICHAEL S. BESSELL Research School of Astronomy and Astrophysics, Institute of Advanced Studies, The Australian National University, Private Bag, Weston Creek P.O., ACT 2611, Australia ; bessell=mso.anu.edu.au Received 2000 March 6 ; accepted 2000 April 17 ABSTRACT. Hipparcos and T ycho magnitudes have been extracted for many of the E-region standard stars. ... B [V regression for the E-region stars. ...

... 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 .. ...

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 ...

... 525 - .099 .096 .224 44937.15830 -. ... 553 - .095 . 096 .221 44937.16670 . 097 44937.16810 . 096 44937.16960 . 090 44937.17110 . 093 44937.17300 .092 44937.17490 . 093 44937.17590 .089 44937.17980 .095 44937.18180 . 093 44937.18330 .100 44937.18480 .089 44937.18620 .092 44937.18770 .095 44937.18960 . 096 44937.19110 .089 44937.19400 . 101 44937.19590 .094 44937.19840 . 101 44937.19980 .100 44937.20130 . 096 44937.20280 .092 44937.20430 . 093 44937.20670 ... 093 . ... 48869.361415 .106 ....

. Proper motions, radial velocities and space motions for pCNS3 late-K and M dwarfs. Astrometric data are primarily from the pCNS3, supplemented by more recent observations where possible; radial velocities are mainly from PMSU1, again updated to include more recently obtained higher-accuracy data (notably from PMSU3). The references are as follows: . 1. from PMSU1 (1018 stars) . 2. from Delfosse, Forveille, Perrier Mayor, 1998, A , 331, 581 (3 stars) . 3. from Tinney Reid, 1998, MNRAS (11 stars) . 4. from

... Source name (L indicates a source within the boundaries of the LMC); (2,3) Source position (position errors are 2.0 sec and 1.1 arcsec in RA and dec respectively); (4,5) Galactic latitude and longitude; (6,7) Source offset from the pointing centre of the 18 GHz followup image; (8,9) 18 GHz peak flux density and its error; (10) Sources which are strongly resolved in the 18 GHz images (i.e. with angular sizes typically 10 ...

. ВНЕСОЛНЕЧНЫЕ ПЛАНЕТЫ: 1199 планетных систем, 2003 планет . Список планет сортируется в зависимости от выбранного Вами пар аметра (например, в зависимости от расстояния планеты от Солнца) . планета . расстояние от Солнца, пк . большая полуось, а.е. масса, m sin i, масс Юпитера . радиус, радиусов Юпитера . орбитальный период, дней . эксцентриситет . аргумент перицентра (омега), град. год открытия . 11 UMi b . 120 . 1.54+0.07 . 10.5+2.5 . - . 516+3 . 0.08+0.03 . 118+21 . 2009 . 14 Andromedae b . 76.4 . 0.83

... Nikolaev 2.8 USNO 094 Russia, Sime- 1.0 6 x 5' 1 1 4 0.541 0.342 iz, INASAN 2.2 USNO 104 Italy, San 0.40 21 x 21' 2.5 21 75 0.235 0.270 Marccello 2.0 GSC 106 Slovenia, 0.36 36 x 36' 2.0 1793 7468 0.315 0.302 Crni vrh 2.4 USNO 114 142 985 0.221 0.173 118 Slovakia, 0.57 14 x 10' 1.7 2 8 0.287 0.357 Modra 3.3 USNO 157 Italy, 0.20 18 x 12' 1.4 14 53 0.205 0.149 Frasso Sabino 1.3 2.8 USNO 212 Obs. ... 1.8 UCAC A24 New Millennium 0.36 12 x 12' 1.4 67 594 0.350 0.254 Obs., ...

May 5, 2006 19:13 Comet R.A. Decl. r d Elong m1 Mot.(') p.a. P/ Schwassmann-Wachmann ( 73P-AA) 15 54 2.57 42 39 27.3 1.063 0.104 119 12.9 146.2 55.9 P/ Schwassmann-Wachmann ( 73P-AB) 16 17 40.30 41 52 50.1 1.060 0.101 118 12.8 167.1 63.3 P/ Schwassmann-Wachmann ( 73P-AC) 16 18 16.80 41 49 11.1 1.060 0.101 118 12.8 167.6 63.5 P/ Schwassmann-Wachmann ( 73P-AD) 16 17 5.20 41 19 27.8 1.063 0.104 118 12.9 161.1 63.9 P/ ...

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

Astronomy & Astrophysics manuscript no. 26199 July 23, 2015 c ESO 2015 Star and jet multiplicity in the high-mass star forming region IRAS 05137+3919 ґ R. Cesaroni1 , F. Massi1 , C. Arcidiacono1,2 , M.T. Beltran1 , P. Persi3 , M. Tapia4 , S. Molinari3 , L. Testi5,1 , L. Busoni1 , 1 , K. Boutsia6 , S. Bisogni7,1 , D. McCarthy8 , and C. Kulesa8 A. Riccardi 1 2 3 4 5 6 7 8 INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy cesa,fmassi,mbeltran,riccardi,lbusoni@arcetri.astro.it

... 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 ...

. *********** FIELD 1 ************* . *********** FIELD 2 ************* . *********** FIELD 3 ************* . *********** FIELD 4 ************* . *********** FIELD 5 ************* . *********** FIELD 6 ************* . *********** FIELD 7 ************* . *********** FIELD 8 ************* . *********** FIELD 9 ************* . *********** FIELD 10 ************* . *********** FIELD 11 ************* . *********** FIELD 12 ************* . *********** FIELD 13 ************* . *********** FIELD 14 ************* .

Mutual Events of the Uranian Satellites, main page . Data in table (text only) . ... Information on events involving Puck and Miranda (unpublished) . The Uranian satellite Puck, imaged by Voyager 2 . The table below contains these columns: . Type of event and satellites involved. ... Distance from uranian limb at onset of event in units of the apparent planetary radius. ... Umb./part. Tot./ann. ... 0.000 . ... 2007 MAR 03 . ... 2007 DEC 02 . ... 2008 JAN 01 . ... 2008 DEC 13 . ...

... 0.0 Azov | ... 180 | ... 189 | ... 176 | ... 0.0 Artem | ... 0.0 Acbest | ... 181 | ... 188 | ... 0.0 Belovo (Kemer.) ... 0.0 Beloretsk | ... 179 | ... 0.0 Bodajbo | ... 0.0 Bol'shoj Kamen' | ... 0.0 | ... 183 | ... 178 | ... 0.0 Vladikavkaz | ... 175 | ... 0.0 Daurskoe | ... 0.0 Ertarskii | ... 0.0 Zlatoust (Cheljab.) ... 0.0 Ivdel' | ... 0.0 Kirovgrad | ... 0.0 Kolpashevo | ... 0.0 Krasnokamsk | ... 0.0 Lys'va (Perm.) ... 0.0 Nazarovo | ... 0.0 Never | ... 0.0 Nevinnomysk | ... 0.0 Neftekamsk | ...

TABLE 1 Baldwin Effect Regressions for the LBQS Emission line All Data (including upper limits) Detections only Line Name N T ot N Limits C/K/S a Slope Intercept N C/K/S a Slope Intercept Fe II UV 953 294 0.00 / 0.00 / 0.00 ­0.617 \Sigma0.047 20.2 \ Sigma 1.4 659 0.00 / 0.00 / 0.00 ­0.105 \ Sigma 0.016 4.8 \ Sigma 0.5 Fe II opt 248 110 0.00 / 0.00 / 0.00 ­0.447 \ Sigma 0.108 14.5 \ ... The Baldwin effect examined here is log L 2500 / log W – (line). ...