{
  "bibcode": "1998GCN...122....1H",
  "body": "SGR 1627-41\n\nK. Hurley, Space Sciences Laboratory, T. Cline, P. Butterworth, NASA\nGSFC, E. Mazets and S. Golenetskii, Ioffe Institute, on behalf of the\nUlysses and Konus-Wind teams, report: \"We have triangulated the\nposition of this soft gamma repeater using 7 Konus-Ulysses events\nbetween 17 and 22 June.   A typical annulus has a center at (equinox\n2000.0) R.A.=22h03m04s, Decl.=-9o49'.8, and a radius 77.247 +/- 0.013\ndegrees.  Around the position of the supernova remnant G337.0-0.1, this\nannulus nests within the one reported previously (IAUC 6948), but is\nconsiderably narrower.  Around this position, the 7 annuli give results\nwhich are mutually consistent to better than 10 arcseconds. The\npositions of the annuli suggest that if the source of the bursts is\nindeed within the SNR, it lies between the two radio lobes.  An image may be\nfound at http://ssl.berkeley.edu/ipn3/sgr1627-41/.  These preliminary\nannuli can be refined further.\"\n\nThis message may be cited.",
  "circularId": 122,
  "createdOn": 899509484000,
  "email": "khurley@sunspot.ssl.berkeley.edu",
  "subject": "SGR1627-41",
  "submitter": "Kevin Hurley at UCBerkeley/SSL  <khurley@sunspot.ssl.berkeley.edu>"
}