Circular No. 3167 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 HDE 245770 C. Bartolini, A. Guarnieri and A. Piccioni, Istituto di Astronomia, Universita di Bologna; and A. Giangrande and F. Giovannelli, Laboratorio di Astrofisica Spaziale, Frascati, report: "On 1977 Dec. 17 and 20 and 1978 Jan. 6 we performed UBV photoelectric photometry of HDE 245770 in order to test our hypothesis on the x-ray flare-up periodicity and the probable related optical emission of the A0535+26-HDE 245770 system. The data, obtained with the 60-cm reflector at Loiano, show significant light enhancement of the star relative to the comparison star BD +26 876 during Dec. 17-20 and successive fading up to Jan. 6. Between Dec. 20.99 and 21.11 UT, about 12 hours after the x-ray flare-up observed by SAS 3 (IAUC 3154), we continuously monitored HDE 245770 and the comparison stars BD +26 876 and BD +25 902. Our results are as follows: 1977/78 UT dU1 dB1 dV1 dU2 dB2 dV2 Dec. 17.12 +1.231 +0.983 20.99 +0.355 +1.205 +0.948 +4.507 +4.409 +3.710 21.11 +0.375 +1.225 +0.960 +4.526 +4.436 +3.728 Jan. 6.87 +0.382 +1.259 +0.981 The differences dU, dB and dV are in the sense HDE 245770 minus comparison star, subscript 1 referring to BD +26 876, subscript 2 to BO +25 902. Standard deviations are 0.009 magnitude on Dec. 17.12, 0.004 on Dec. 20.99 and 21.11, 0.015 on Jan. 6.87. Between the first and last times it appears that the observed B-V of HDE 245770 increased by about 0.03 magnitude. The observed enhancement of optical emission during the flare-up of the x-ray source gives a direct argument strongly supporting identification of HDE 245770 with A0535+26, a transient x-ray source with double eruptive events separated by about 200 days and probably recurring with a period of about 765 days." PERIODIC COMET GIACOBINI-ZINNER The following ephemeris, by D. K. Yeomans, is from Handb. Br. Astron. Assoc. for 1978: For dT = +1d 1978 ET R. A. (1950) Decl. Delta r dR.A. dDecl. Mag. Apr. 2 16 15.90 + 2 27.9 2.754 3.440 -0m64 - 1'7 21.1 12 16 13.29 + 4 19.8 -0.68 - 2.0 22 16 08.50 + 6 17.5 2.450 3.304 -0.71 - 2.4 20.6 May 2 16 01.64 + 8 15.7 -0.73 - 2.9 12 15 53.01 +10 07.3 2.245 3.163 -0.74 - 3.4 20.3 22 15 43.20 +11 45.0 -0.73 - 4.0 June 1 15 32.95 +13 02.3 2.150 3.016 -0.71 - 4.5 20.0 11 15 23.12 +13 54.5 -0.67 - 4.9 21 15 14.54 +14 20.2 2.151 2.863 -0.63 - 5.1 19.7 July 1 15 07.84 +14 20.4 -0.58 - 5.2 11 15 03.44 +13 58.1 2.213 2.705 -0.54 - 5.2 19.5 21 15 01.56 +13 17.2 -0.51 - 5.0 31 15 02.23 +12 21.6 2.299 2.541 -0.48 - 4.7 19.4 Aug. 10 15 05.40 +11 14.8 -0.47 - 4.4 20 15 10.96 + 9 59.9 2.375 2.371 -0.47 - 4.1 19.1 30 15 18.78 + 8 39.4 -0.48 - 3.7 Sept. 9 15 28.77 + 7 15.3 2.421 2.195 -0.50 - 3.2 18.8 19 15 40.86 + 5 49.5 -0.54 - 2.8 29 15 54.99 + 4 23.2 2.424 2.013 -0.58 - 2.3 18.5 Oct. 9 16 11.18 + 2 58.1 -0.64 - 1.8 19 16 29.47 + 1 35.4 2.381 1.828 -0.71 - 1.2 18.0 29 16 49.92 + 0 16.5 -0.81 - 0.7 Nov. 8 17 12.67 - 0 57.1 2.295 1.640 -0.91 - 0.1 17.5 18 17 37.82 - 2 03.8 -1.04 + 0.5 28 18 05.53 - 3 02.0 2.179 1.454 -1.20 + 1.1 16.8 PERIODIC COMET WILD 2 (1978b) P. Wild, Astronomical Institute, Berne University, provides further precise positions as follows: 1978 UT R. A. (1950) Decl. Jan. 25.73403 5 19 00.02 +19 53 16.9 25.75556 5 18 59.12 +19 53 21.1 The following orbital elements, by B. G. Marsden, indicate that this is a short-period comet that passed very close to Jupiter in 1974. Wild also remarks on the comet's short period. T = 1978 June 14.90 ET Peri. = 39.48 e = 0.5566 Node = 136.33 1950.0 a = 3.3583 AU Incl. = 3.26 n = 0.16015 q = 1.4891 AU P = 6.15 years 1978 ET R. A. (1950) Decl. Delta r m1 Jan. 22 5 21.18 +19 46.0 Feb. 1 5 16.61 +20 07.5 1.232 1.999 13.5 11 5 16.24 +20 34.2 21 5 20.23 +21 05.3 1.309 1.881 13.3 Mar. 3 5 28.39 +21 38.5 13 5 40.44 +22 10.7 1.401 1.771 13.2 1978 January 30 (3167) Brian G. Marsden
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