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Observations of a Possible New Soft Gamma Repeater, SGR 1801–23

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© 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation T. Cline et al 2000 ApJ 531 407 DOI 10.1086/308470

0004-637X/531/1/407

Abstract

We report on two 1997 June observations of a soft bursting source whose time histories and energy spectra are consistent with those of the soft gamma repeaters. The source can be localized only to an ≈3fdg8 long error box in the direction of the Galactic center, whose area is ≈80 arcmin2. The location of the source, while not consistent with that of any of the four known soft repeaters, is consistent with those of several known and possible supernova remnants.

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10.1086/308470