QPOs in Accreting Pulsars

Details QPOs in Accreting Pulsars QPOs in Accreting Pulsars

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..714..342f&link_type=abstract

X-RAY TIMING 2003: Rossie and Beyond. AIP Conference Proceedings, Volume 714, pp. 342-345 (2004).

Computer Science

2

Pulsars, X-Ray

Scientific paper

Quasi-Periodic phenomena has been seen in several types of long-period (P > 50 ms) accreting pulsars, including the Be/X-ray transients and the super-giant disk-fed systems. It has also been seen in the ultra-compact LMXB system 4U 1626-67, and the unique LMXB transient GRO J1744-28. I summarize these observations, and discuss what can be learned from observing with an instrument more sensitive than RXTE/PCA.

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