Search for timing glitches in the non-burst emission from GRO J1744-28

Details Search for timing glitches in the non-burst emission from GRO J1744-28 Search for timing glitches in the non-burst emission from GRO J1744-28

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20718318h&link_type=abstract

American Astronomical Society Meeting 207, #183.18; Bulletin of the American Astronomical Society, Vol. 37, p.1471

Astronomy and Astrophysics

Astronomy

Scientific paper

GRO J1744-28 is one of only a handful of X-ray pulsars for which accurate, phase-connected pulse timing is available over a period of years. Recent reports of possible glitches in othe X-ray pulsar data caused us to reexamine the archival RXTE data of this source. There are a few events which are interesting in terms of the possiblity of sudden changes in the pulsar frequency independent of accretion onto the star. We present a study of the relationship between accretion and frequency change for this source and highlight the interesting events.

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