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IAUC 4585: AE Aqr; 1988b; N LMC

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                                                  Circular No. 4585
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
TWX 710-320-6842 ASTROGRAM CAM    Telephone 617-495-7244/7440/7444
MARSDEN or GREEN@CFA.BITNET    MARSDEN or GREEN@CFAPS2.SPAN


AE AQUARII
     K. Horne and R. McCray, Space Telescope Science Institute,
communicate: "Simultaneous x-ray, ultraviolet, optical and radio
observations of the dwarf nova AE Aqr (R.A. = 20h37m34s.3, Decl. =
-1d02'57", equinox 1950.0; V = 10-12) are scheduled for June to study
the physical processes responsible for the 16 and 32 s pulsations and
violent flickering seen in this accreting binary.  Ginga will observe
AE Aqr from June 2d02h through June 4d08h UT.  IUE coverage will begin
on June 2d05h and end on June 3d21h.  VLA will observe at the same
time as IUE (when the source is up). Time-resolved photometry or
spectroscopy in the optical or infrared would be extremely valuable
during this time.  Potential observers wishing additional information
should contact us at HORNE@SCIVAX.SPAN or MCCRAY@SCIVAX.SPAN."


COMET SHOEMAKER (1988b)
     Improved parabolic orbital elements from MPC 12952:

     T = 1987 Mar. 19.461 ET          Peri. = 124.124
                                      Node  = 324.488   1950.0
     q = 5.02568 AU                   Incl. =  80.508

     1988 ET      R.A. (1950) Decl.     Delta      r       m1
     Apr. 29     9 14.51    +27 28.3    5.730    5.891    14.0
     May   9     9 13.87    +26 16.2
          19     9 14.42    +25 04.1    6.135    5.969    14.2
          29     9 15.99    +23 52.6
     June  8     9 18.41    +22 41.7    6.520    6.050    14.4
          18     9 21.53    +21 31.6
          28     9 25.20    +20 22.1    6.856    6.132    14.6

     Total visual magnitude estimate by D. Levy, Tucson, AZ (Catalina
1.54-m reflector): Apr. 9.29 UT, 13.8.  There was a possible tail 2'
long in p.a. 310 deg).


NOVA IN THE LARGE MAGELLANIC CLOUD
     Visual magnitude estimates by R. H. McNaught, Coonabarabran,
N.S.W.: Apr. 13.55 UT, 13.3; 14.52, 13.4; 15.48, 13.4; 18.44, 13.4:;
19.50, 13.1; 20.42, 13.5; 22.43, 13.6; 22.54, 13.2.


1988 April 23                  (4585)              Brian G. Marsden

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