The Pulsar in GRO J1744-28 at Low Flux

Details The Pulsar in GRO J1744-28 at Low Flux The Pulsar in GRO J1744-28 at Low Flux

1997-12-11

arxiv.org/abs/astro-ph/9712154v1

1998, in Accretion Processes in Astrophysical Systems: Some Like It Hot!, ed. S. S. Holt & T. R. Kallman (AIP Conf. Proc. 431)

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, AIP Proceedings LaTex format, to appear in "Accretion Processes in Astrophysical Systems", Proc. of the 8t

Scientific paper

10.1063/1.55877

The Bursting Pulsar, GRO J1744-28, has been observed with the Rossi X-ray Timing Explorer (RXTE) regularly since the launch of the satellite in December 1995. This accretion driven pulsar has undergone two outbursts which have been accompanied by significant spin-up of the pulsar. Between these two outbursts, the pulsar was detectable during each observation down to fluxes perhaps one thousandth of the persistent flux at the peak of the first outburst. We observe evidence of a change in the sign of the frequency derivative during the faintest period but the relationship between the observed luminosity and the frequency derivative is complex.

Affiliated with

Also associated with

No associations

Rating

The Pulsar in GRO J1744-28 at Low Flux does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Pulsar in GRO J1744-28 at Low Flux, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Pulsar in GRO J1744-28 at Low Flux will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-527195