Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 3167: HDE 245770; P/GIACOBINI-ZINNER; 1978b

The following International Astronomical Union Circular may be linked-to from your own Web pages, but must not otherwise be redistributed (see these notes on the conditions under which circulars are made available on our WWW site).


Read IAUC 3166  SEARCH Read IAUC 3168
IAUC number


                                                  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 3166  SEARCH Read IAUC 3168


Our Web policy. Index to the CBAT/MPC/ICQ pages.


Valid HTML 4.01!