Circular No. 2830 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 Western Union: RAPID SATELLITE CAMBMASS NOVA CYGNI 1975 The following photoelectric magnitudes have been reported: 1975 UT V B - V U - B V - R R - I b - y Observer Aug. 30.3 1.98 +0.51 -0.81 +0.57 +0.15 Strittmatter 30.40 2.01 +0.40 Fawley 30.52 2.02 " 31.25 1.92 +0.64 -0.11 Schommer 31.3 1.87 +0.62 -0.65 +0.82 +0.21 Strittmatter 31.33 1.90 +0.64 +0.02 Tedesco 31.51 2.02 +0.65 -0.15 Schommer Sept. 1.3 2.26 +0.55 -0.69 +1.03 +0.20 Strittmatter 1.31 2.61 +0.49 -0.21 Tedesco 1.47 2.80 +0.49 -0.40 Schommer 2.18 3.73 +0.34 -0.52 " 2.19 3.96 +0.38 Fawley 2.32 4.19 +0.35 " 2.38 4.24 +0.34 " 2.47 4.02 +0.31 -0.54 Schommer P. A. Strittmatter et al. (University of Arizona). W. Fawley (University of California, Berkeley). R. Schommer and J. Deeter (University of Washington). From the extremely rapid decline G. Wallerstein deduces M_v = -9.2. E. F. Tedesco, A. Herzog, T. Schneeberger and G.Garwood(New Mexico State University). Comparison star epsilon Cyg. Errors ~ +/- 0.02. The following recent visual magnitude estimates have been reported: Sept. 3.07, 4.2 (C. Sherrod, North Little Rock, Arkansas); 3.10, 3.7 (D. di Cicco, Waltham, Massachusetts); 3.21, 4.8 (Sherrod); 4.07, 4.8 (L. Jacchia, Cambridge, Massachusetts); 4.08, 4.9 (Sherrod); 4.10, 4.7 (di Cicco). A0620-00 P. R. Warren, South African Astronomical Observatory, reports: "Blue band observations made by Robertson using the 51-cm telescope at Sutherland on Aug. 22, 23, 24 and 25 UT for periods of about 1.5 hr and with time resolution of about 3 min show the optical candidate for A0620-00 to have an approximately constant B magnitude of 11.3, but to show variations of 0.1 magnitude on time scales of between 30 and 60 min. B-V values ranged between +0.05 and +0.70." 1975 September 4 (2830) Brian G. Marsden
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