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A Second Glitch from the "Anomalous" X-Ray Pulsar 1RXS J170849.0-4000910
Author(s) -
V. M. Kaspi,
F. P. Gavriil
Publication year - 2003
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/379093
Subject(s) - glitch , pulsar , astrophysics , physics , astronomy , optics , detector
We report on 5.4 yr of phase-coherent timing, using the Rossi X-ray TimingExplorer, of the X-ray pulsar 1RXS 1708-4009, a member of the class known as``anomalous X-ray pulsars.'' This object exhibited a rotational glitch in 1999.Here we report a second much larger rotational glitch which occured ~1.5 yrafter the first. We show that the recoveries from the two glitches aredifferent, with the first showing only a possible slow, approximately linearrecovery, while the second showed a nearly complete recovery on a time scale of\~50 days. The approximately exponential recovery time scale of the secondglitch is similar to that seen recently in 1E 2259+586 at the time of a majoroutburst. This suggests 1RXS 1708-4009 undergoes similar bursting behavior,although with our sparse observations we have detected no other evidence forbursts from this source.Comment: 13 pages, 2 figures. Revised manuscript and Fig 1 following refereeing. Accepted for publication in ApJL Aug 1

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