A0586 07 32 17.8 +31 37 34 0.1710 # Probably fainter from twin nuclei in common envelope of brightest galaxy # (similar cD in merging) is identified with radio source in cluster center (RG1). Radio galaxy (RG2) can be in cluster as and 2 nonidentified diffused # NVSS (WENSS) radio sources. ... NVSS (and WENSS) radio source is similar on the tail of HT radio galaxy. Also there is once more extended radio source: # nvss 07 32 27.81 +31 42 40.2 15.8 127.3 44.2 51.3 # which lefts in WENSS. ...
Statistics of sunspot activity . The sunspot indices . ... NGDC's observations . The solar regions . ... Average annual indices . January . ... January, 1990 . Visual indices of solar activity by National Geophysical Data Center . ... Average . ...
... ESO, the European Southern Observatory . ... ESO's Governing Bodies . ... Travel to ESO Headquarters . ... Travel to Chajnantor . ... Visits to ESO Sites . ... Architecture at ESO . ... Green ESO . ... Images . ... 2007 . ... Usage of ESO Images and Videos . ... Usage of ESO Videos and Images . ... ESOshop . ... Mounted Images . ... Mounted images . ... The heart of the ALMA antenna array will be located close to the centre of this image, though the 66 separate antennas will spread over the plateau....
Computer Ephemeris for 2014 from DE200/LE200. Ephemeris for physical observation of the Sun. Date P B L Date P B L Jan 0 2.58 -2.88 202.62 Feb 1 -12.13 -6.01 141.25 1 2.09 -3.00 189.45 2 -12.53 -6.08 128.09 2 1.61 -3.12 176.28 3 -12.93 ... Date P B L Date P B L Jul 1 -2.75 2.84 320.71 Aug 1 10.76 5.76 270.52 2 -2.29 2.95 307.47 2 11.15 5.84 257.29 3 -1.84 3.06 294.23 3 11.55 5.91 244 ...
SOURCE.T - Custom source talogue for use by the program VLBI Modes: 0 X,Y 8 Ra, Dec (J2000) 2 Az,El 10 Ra, Dec (B1950) 4 Ha, Dec 12 l,b 6 Ra, Dec (date) +++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ + DO NOT USE TAB CHARACTERS IN THIS SOURCE LIST + + Please ... ++++++++++++++++++++++ Name Mode Left Right Date Valid Comments/Origin ---- ---- ---- ----- ---------- --------------- ZENITH 0 000 00 00.00 -02 00 00.00 1900 000 SPOLE 4 00 00 ... TH-program (eking) ...
... We detected outbursts in seven systems, one of which (SDSS J0129) was seen in outburst for the first time. ... Of the 18 AM CVn systems in our LT survey, c 0000 RAS, MNRAS 000, 000000 seven were found to show at least one outburst (CR Boo, KL Dra, SDSS J0926, CP Eri, V406 Hya, SDSS J0129 and SDSS J0804). ... 3.6 CP Eri 3.9 SDSS J0804 Of all our `outbursting' AM CVn systems, SDSS J0804 shows the lowest amplitude variations (1.2 mag) and has the longest orbital p eriod. ...