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Circular No. 7040
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
Mailstop 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS@CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
BMARSDEN@CFA.HARVARD.EDU or DGREEN@CFA.HARVARD.EDU (science)
URL http://cfa-www.harvard.edu/iau/cbat.html
Phone 617-495-7244/7440/7444 (for emergency use only)
COMET C/1998 U3 (JAGER)
Ninety-one precise positions that appear on MPEC 1998-U26,
spanning Oct. 24-27, yield the following preliminary parabolic
orbital elements. This comet is likely of short period.
T = 1998 Dec. 9.919 TT Peri. = 138.252
Node = 313.194 2000.0
q = 2.66631 AU Incl. = 17.842
1998 TT R. A. (2000) Decl. Delta r Elong. Phase m1
Oct. 14 6 31.93 +41 23.7 2.323 2.733 103.5 20.8 12.7
19 6 37.90 +41 28.6 2.258 2.722 107.0 20.5 12.6
24 6 43.29 +41 32.4 2.195 2.712 110.7 20.1 12.5
29 6 48.03 +41 35.0 2.135 2.703 114.5 19.5 12.5
Nov. 3 6 52.10 +41 36.3 2.077 2.694 118.4 18.9 12.4
8 6 55.46 +41 36.3 2.022 2.687 122.4 18.1 12.3
13 6 58.07 +41 34.9 1.971 2.681 126.6 17.2 12.3
18 6 59.89 +41 31.6 1.923 2.676 130.9 16.2 12.2
23 7 00.93 +41 26.3 1.879 2.672 135.2 15.1 12.1
28 7 01.19 +41 18.5 1.840 2.669 139.7 13.8 12.1
Dec. 3 7 00.72 +41 07.7 1.805 2.667 144.2 12.5 12.0
8 6 59.56 +40 53.7 1.775 2.666 148.6 11.1 12.0
13 6 57.79 +40 35.9 1.752 2.667 153.0 9.6 12.0
Total visual magnitude and coma-diameter estimates: Oct. 26.01
UT, 12.2, 1'.7 (K. Hornoch, Lelekovice, Czech Republic, 0.13-m
reflector); 26.42, 12.3, 2' (A. Hale, Cloudcroft, NM, 0.41-m
reflector); 26.97, 12.3, 1'.5 (R. J. Bouma, Groningen, The
Netherlands, 0.25-m reflector); 27.17, 12.3, 1'.0 (A. Pereira, Cabo
da Roca, Portugal, 0.25-m reflector).
AX J0049-732
K. Imanishi, J. Yokogawa, and K. Koyama, Kyoto University,
write: "An ASCA observation made on 1997 Nov. 13 detected x-ray
pulsations with a period of 9.1321 +/- 0.0004 s from a source at
R.A. = 0h49m23s, Decl. = -73o12'38" (equinox 2000.0; +/- 1' at
90-percent confidence), designated as AX J0049-732. The x-ray
flux at 2-10 keV was about 8 x 10E-13 erg sE-1 cmE-2."
(C) Copyright 1998 CBAT
1998 October 27 (7040) Daniel W. E. Green
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