**** System Temperature Log **** Log started: 309 5-NOV-1998 08:37:15 UT Cal size used (A): 1.00 (B): 1.00 **** System Temperature Log **** Log started: 309 5-NOV-1998 08:38:26 UT Cal size used (A): 1.00 (B): 1.00 **** System Temperature Log **** Log started: 309 5-NOV-1998 08:39:13 UT Cal size used (A): 1.00 (B): 1.00 **** System Temperature Log **** Log started: 309 5-NOV-1998 08:41:41 UT Cal size used (A): 1.00 (B): 1.00 **** System Temperature Log **** Log started: 309 5-NOV-1998 08:52:02 UT Cal size
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
fk5 ; box (17:46:07.510,-28:59:51.20,12 ,1 ) # color = red width =1 text ={@87556} fk5 ; box (17:45:11.510,-29:02:36.80,12 ,1 ) # color = red width =1 text ={@78390} fk5 ; box (17:45:19.900,-29:05:12.30,12 ,1 ) # color = blue width =1 text ={@69015} fk5 ; box (17:45:46.930,-29:04:08.50,12 ,1 ) # color = blue width =1 ...
Computer Ephemeris for 2014 from DE200/LE200. Reduction quantities ( dynamical time scale). tau A+A' B+B' C D E A' B' a 0s0001 0 001 0 001 Jan 1 -0.5000 -5.888 8.279 -3.493 20.488 14 16 88 2 -0.4973 -5.772 8.253 -3.823 20.418 14 63 65 3 -0.4945 -5.674 8.209 -4.152 20 tau A+A' B+B' C D E A' B' a 0s0001 0 001 0 001 Feb 1 -0.4151 -3.903 7.810 -12.669 15.552 15 88 -44 2 -0.4124 -3.876 7.764 -12.915 15.304 15 63 -74 3 -0.4097 -3.860 7.739 -13.157 ...
... Received 2008; in original form 2008 ABSTRACT The rapidly oscillating Ap (roAp) star 10 Aql shows one of the lowest photometric pulsation amplitudes and is characterized by an unusual spectroscopic pulsational behavior compared to other roAp stars. ... The dramatic decline of pulsations in the atmospheric layers probed by the strong Pr III and Nd III lines accounts for the apparent peculiarity of 10 Aql when compared to other roAp stars. ... Pulsations in the roAp star 10 Aql Table 6. ...
Peremennye Zvezdy ( Variable Stars ) 28 , No. ... We present a list of 109 probable RS CVn variables among stars in the ASAS-3 catalog with Population II Cepheid classification as the main one or an alternative one. These stars are identified with X-ray sources and have light curves (from ASAS-3 data) in no contradiction with the suggested RS CVn classification. ... Among stars we were able to identify with known X-ray sources of the following catalogs: 1RXS (Voges et al. ... ASAS-3 . ... NSV . ...