Read IAUC 3168
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
Read IAUC 3168
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