Read IAUC 5351
Circular No. 5350
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Postal Address: Central Bureau for Astronomical Telegrams
Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
Telephone 617-495-7244/7440/7444 (for emergency use only)
TWX 710-320-6842 ASTROGRAM CAM EASYLINK 62794505
MARSDEN or GREEN@CFA.BITNET MARSDEN or GREEN@CFAPS2.SPAN
1991 RC
Further precise positions have been reported as follows:
1991 UT R.A. (1950) Decl. V Observer
Sept.13.54492 21 57 13.22 -11 12 27.5 18.5 Hartley
17.19326 21 49 19.90 -12 28 05.2 Scotti
17.20201 21 49 18.81 -12 28 15.2 "
17.21062 21 49 17.70 -12 28 25.0 "
M. Hartley (Siding Spring). 1.2-m U.K. Schmidt. Beginning of
faint trail. Measurer R. H. McNaught.
J. V. Scotti (Kitt Peak). 0.91-m Spacewatch telescope.
Improved elements, from the eight observations Sept. 3-17, show
that the orbit is very similar to that of (1566) Icarus:
T = 1991 Apr. 23.613 ET Peri. = 8.161
e = 0.82871 Node = 160.645 1950.0
q = 0.18536 AU Incl. = 23.543
a = 1.08214 AU n = 0.875551 P = 1.13 years
1991 ET R.A. (1950) Decl. Delta r V
Sept.11 22 03.27 -10 14.7 0.859 1.843 18.6
16 21 51.81 -12 04.2
21 21 42.09 -13 37.5 0.962 1.882 19.2
26 21 34.14 -14 55.3
Oct. 1 21 27.88 -15 59.1 1.090 1.914 19.7
6 21 23.21 -16 50.3
11 21 19.99 -17 30.6 1.234 1.940 20.1
AM HERCULIS
H. Jessop, Sonoma State University; and P. A. Mason, Louisiana
State University, report that AM Her remains in its low accretion
state (cf. IAUC 5312). Cooled CCD observations made with the Sonoma
State University 0.17-m telescope indicate that AM Her was at V = 15.1
(orbital average) and that it did not vary from this average by more
than 0.2 mag during 3.2 hr of 1-min integrations. The observations
were centered on Sept. 5.24 UT, and the result is consistent with low-
state behavior.
1991 September 18 (5350) Brian G. Marsden
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