Central Bureau for Astronomical Telegrams

Central Bureau for Astronomical Telegrams -- Image credits

IAUC 8341: 2004bs, 2004bt; C/2003 Q10, T9-T11, U5, U6, W2, Y1

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 8340  SEARCH Read IAUC 8342

View IAUC 8341 in .dvi or .ps format.
IAUC number


                                                  Circular No. 8341
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)
CBAT@CFA.HARVARD.EDU (science)
URL http://cfa-www.harvard.edu/iau/cbat.html  ISSN 0081-0304
Phone 617-495-7440/7244/7444 (for emergency use only)


SUPERNOVAE 2004bs AND 2004bt
     Further to IAUC 8336, M. Armstrong reports his discovery of an
apparent supernova (mag 17.0) on unfiltered CCD images taken on May
16.914 and 17.884 UT.  SN 2004bs is located at R.A. = 10h39m39s.30,
Decl. = +25o19'19".9 (equinox 2000.0), which is approximately 3".4
east and 1".7 south of the center of NGC 3323.  Nothing was visible
at this position on his images taken on 2000 Dec. 22 (limiting mag
about 19.5), 2004 Apr. 13, 19, and 25 (limiting mag about 19) or on
Palomar Sky survey red and blue plates.
     Further to IAUC 8311, T. Boles reports the discovery of an
apparent supernova (mag 18.2) on unfiltered CCD images taken on May
17.023 and 18.001 UT.  The new object is located at R.A. =
14h19m53s.88, Decl. = +51o53'49".6, which is approximately 6".3
west and 8".1 north of the center of UGC 9178.  SN 2004bt is not
present on Boles' images from Mar. 22 and Feb. 20 (limiting mag
19.5), and it is not present on Digitized Sky Survey red (1994) or
blue (1995) plates.


COMETS C/2003 Q10, T9-T11, U5, U6, W2, Y1 (SOHO)
     Further to IAUC 8340, K. Battams reports measurements for
additional near-sun comets found on SOHO website images by M.
Boschat (C/2003 Q10, T11), X.-m. Zhou (C/2003 T9, W2), J. Sachs
(C/2003 T10), X. Leprette (C/2003 U5), and M. Meyer (C/2003 Y1).
C/2003 Q10 was observed only in C3 images, while C/2003 T9, T11,
U5, and W2 were observed only in C2 images; the remaining comets
were observed in both coronagraphs.  The reduced astrometry by
B. G. Marsden and R. Kisala, and orbital elements by Marsden,
appear on the MPECs cited below.  C/2003 W2 and C/2003 Y1 belong to
the Meyer group; the remaining objects are Kreutz sungrazers.

  Comet         2003 UT          R.A. (2000) Decl.       MPEC
  C/2003 Q10    Aug. 25.113       9 57.0   +10 29       2004-K16
  C/2003 T9     Oct.  9.746      12 51.1   - 6 48       2004-K16
  C/2003 T10    Oct. 13.404      12 49.8   - 9 16       2004-K16
  C/2003 T11    Oct. 15.479      13 12.5   - 9 12       2004-K16
  C/2003 U5     Oct. 16.996      13 18.0   - 9 46       2004-K16
  C/2003 U6     Oct. 20.638      13 20.9   -12 04       2004-K16
  C/2003 W2     Nov. 29.379      16 19.3   -23 07       2004-J21
  C/2003 Y1     Dec. 20.379      17 52.3   -22 21       2004-J21

                      (C) Copyright 2004 CBAT
2004 May 18                    (8341)            Daniel W. E. Green

Read IAUC 8340  SEARCH Read IAUC 8342

View IAUC 8341 in .dvi or .ps format.


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


Valid HTML 4.01!