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IAUC 3178: 1978a; AX Per

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                                                  Circular No. 3178
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


COMET WEST (1978a)
     The following precise positions have been reported:

     1978 UT             R. A. (1950) Decl.        m1    Observer
     Jan. 19.86319    14 31 22.06   -12 57 51.5  16-16.5 Seki
     Feb.  6.77014    14 30 41.59   -11 03 44.3   16       "
           6.79758    14 30 41.33   -11 03 34.7            "
           8.32407    14 30 26.84   -10 52 20.5          Schuster

T. Seki (Kochi Observatory, Geisei Station).  40-cm reflector.
   From Orient. Astron. Assoc. Comet Bull. Nos. 160 and 162.
H.-E. Schuster (European Southern Observatory).  Measurer: R. M. West.
   100-cm Schmidt telescope.  Partially overlaps star.

     Extension of the ephemeris on IAUC 3165:

     1978 ET     R. A. (1950) Decl.     Delta     r      m1
     Mar. 13    14 18.11    - 5 58.7    5.088   5.853   16.7
          23    14 11.81    - 4 11.5
     Apr.  2    14 04.66    - 2 19.9    4.949   5.895   16.7
          12    13 56.94    - 0 27.5
          22    13 49.02    + 1 22.0    4.957   5.940   16.7
     May   2    13 41.26    + 3 05.0
          12    13 34.00    + 4 38.6    5.116   5.987   16.8
          22    13 27.53    + 6 00.7
     June  1    13 22.05    + 7 10.7    5.399   6.038   17.0
          11    13 17.68    + 8 08.4
          21    13 14.47    + 8 54.6    5.761   6.092   17.1
     July  1    13 12.42    + 9 30.5
          11    13 11.47    + 9 57.5    6.156   6.148   17.3

            m1 = 5.5 + 5 log Delta + 10 log r


AX PERSEI
     J. Bortle, Brooks Observatory, and S. O'Connor, Montreal, Quebec,
have independently reported that this Z And variable is having
an outburst.  Visual magnitude estimates: Jan. 17.0, 9.2 (Bortle);
29.0, 9.3 (Bortle); Feb. 9.0, 9.4 (Bortle); 13.1, 9.1 (O'Connor).
J. Mattei informs us that AAVSO observations show the magnitude to
have varied only between 11.4 and 12.9 since 1969 and that the star
seems still to have been faint at the beginning of Jan. 1978.


1978 February 24               (3178)              Brian G. Marsden

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