Circular No. 3013 Central Bureau for Astronomical Telegrams INTERNATIONAL ASTRONOMICAL UNION Postal Address: Central Bureau for Astronomical Telegrams Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A. Cable Address: SATELLITES, NEWYORK Telex: 921428 Telephone: (617) 864-5758 X-RAY SOURCES M. G. Watson, J. Pye, M. Elvis and A. Lawrence, X-Ray Astronomy Group, University of Leicester, report that observations during the Ariel 5 galactic plane scan (cf. IAUC 2995) showed Cir X-1 to become visible on Nov. 24 and to increase in intensity to approximately 90 Ariel cts/s (~ 240 Uhuru cts/s); the intensity dropped sharply on Nov. 26.4 UT, approximately in phase with the prediction by Kaluzienski et al. (see also IAUC 3003). A new, variable source has appeared near the galactic center at ~ 7 Ariel cts/s with line of position centered on R.A. = 18h05m.5, Decl. = -18o37' (equinox 1950.0). A source with ~ 40 cts/s is present with line of position near 3U 1727-33 and possibly associated with MXB1730-335 in its 'on' state. VV CEPHEI I. D. Howarth, Department of Physics and Astronomy, University College, London, provides the following observations, confirming that the eclipse has begun: Nov. 3.9 UT, V = 4.87, B = 6.84; Nov. 22.9, V = 5.13, B = 7.08, U = 8.52. With further reference to the note on IAUC 3006, A. Galatola suggests that 20 Cep be used for the comparison star and that each observer determine its photometric parameters in his own telescope system. COMET LOVAS (1976k) T. Seki, Kochi Observatory, Geisei Station, provides the following precise positions, obtained using a 40-cm reflector: 1976 UT R. A. (1950) Decl. Nov. 23.72361 9 20 21.4 +72 12 42 23.79410 9 20 15.7 +72 12 55 1973 NA J. Gibson provides the following precise position, measured from a plate taken with the 51-cm double astrograph at the former Yale-Columbia Southern Station, El Leoncito: 1973 UT R. A. (1950) Decl. Aug. 1.03472 14 36 26.93 -64 25 32.0 1976 December 1 (3013) Brian G. Marsden
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