272 Prog RA De X rg WF 123 CFN A WHS FN VI C Special Reqs L O sta PC 12065A8 18 sc 1 11.016:21 11.018:21 2 1 -S S.------ --S v 111 GO 42 -4 e F NN NNN NNN N YNN NN PP - S4+7= L - re PER 12065A9 18 sc 1 11.016:21 11.018:23 2 1 -S S.------ --S v 111 GO 42 -4 e F NN NNN NNN N PNN NN NY - S4= L - re PER 12061CM 18 sc 1 11.014:12 11.019:10 5 1 -S .------- --- v 111 GO 53 -28 e F NN NNN NNN N ... re VIC 1232421 18 sc 1 11.017:00 11.024:00 6 2 -. ...
This page is devoted to information on Supernova 1999gi in NGC 3184 . ... Information on the original web pages for many of these images can be found on the Supernova links web page. ... NGC 3184 is a fairly close Mag 10.3 galaxy, only about half as distant as the Virgo cluster. ... Seiichi Yoshida has a 1999gi page . Odd Trondal's 1999gi page . ... CfA image . ... 14.5 . ... Jean Marie Llapasset image . ... vsnet-alert 3805 ] SN 1999gi in NGC 3184 . vsnet-chat 2438 ] Host galaxy of SN1999gi . ...
... 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 . ...
... 5-GHz total flux density . ... EW position (mas) . ... 0.2 .. ... Other VLBI references . 2.3 and/or 8.4 GHz: multiple epoch VLBI images are available in the USNO Radio Reference Frame Image Database (RRFID, Fey & Charlot 2000, ApJS 128, 17) . 15 GHz: multiple epoch VLBI images are available in the USNO Radio Reference Frame Image Database (RRFID, Fey & Charlot 2000, ApJS 128, 17) . 15 GHz: multiple epoch VLBI images are available in the VLBA 2-cm survey (Kellermann et al. ...
. Tabella B1 (in EURO ) . (vedi Tabella in Lire ) . STIPENDI TABELLARI . (in euro per 12 mensilitЮ) . Livello . dal 1.11.98 . Ispettore Generale r.e. 17.150,68 . Direttore Divisione r.e. 15.585,50 . Quarto livello . 12.753,90 . Quinto livello . 11.033,07 . Sesto livello . 9.630,37 . Settimo livello . 8.337,16 . Ottavo livello . 7.536,65 . Nono livello . 6.882,82 . Decimo livello . 6.235,18 .
SN/PSN=SuperNovae, DN - Dwarf Nova (UG), ATel= TheAstronomer'sTelegramms , GCN =Gamma-ray bursts Center Network Circulars; MASTER observatories, where these transients were discovered: Amu= MASTER-AMUR , Tun= MASTER-TUNKA , Kis MASTER-Kislovodsk , SA= MASTER-SAAO(SouthAfrica, Sutherland) , IAC= MASTER-IAC (Teyde Observatory of Instituto di Astrofisica di Canarias), Arg=MASTER-Argentina, Dom=MASTER-Domodedovo The Principal Investigator is Professor Vladimir Lipunov MASTER is supported by The Development
Тема : Хвостатые гостьи V (информация для наблюдения комет) .. Показать сообщение отдельно . ... Re: Хвостатые гостьи (информация для наблюдения комет) .. ... Элементы орбиты кометы C/2010 G2 (Hill): . ... Эфемериды для поиска кометы C/2010 G2 (Hill) на московском небе на 24:00 мск.: ... Карта движения кометы C/2010 G2 (Hill) в сентябре 2011 года .. ...
... Nova M81 2004 4 , Unannounced discovered 2004/09/15.280 by K. Hornoch . ... Located 53.9" east and 14.2" south of the center of NGC 3031 (= M81 ) ( Discovery image ) . ... Nova M31 2004 24 , Unannounced, discovered 2004/12/21.856 by Kamil Hornoch . ... Located 183.6" west and 372.9" south of the center of NGC 224 (= M31 ) ( Discovery image ) . ... Nova M31 2004 23 , Unannounced, discovered 2004/11/29.796 by Kamil Hornoch . ... Nova M31 2004 14 , Unannounced, discovered 2004/07/30.00 by Marco Fiaschi...
... In recent years, substantial information concerning the Io torus has been published. ... Explaining the observed steady state rotation of the torus seems to be difficult. The angular velocity of the torus must be in accordance with the celestial mechanics laws, of the same orders as Io's one. ... We wish to straighten out the situation describing the main geometric and kinematic features of the Io torus using a steady state model based on some of Alfven's ideas [Alfven, 1981]. ...
Astronomy & Astrophysics manuscript no. chamcompanions November 29, 2011 c ESO 2011 Discarded candidate companions to low-mass members of Chamaeleon I (Research Note) Д F. Comeron1 ? ... We study two faint objects at a very small angular distance from the low-mass star ESO-H-558 and the possible massive brown dwarf ESO-H-566, both of which are members of the Chamaeleon I star-forming region, to establish whether they are physical companions to those sources. ... 2004), ESO-H-558 and ESO-H-566. ...