Long-term RXTE monitoring of the anomalous X-ray pulsar 1E 1048.1–5937
Author(s) -
V. M. Kaspi
Publication year - 2001
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.177
H-Index - 75
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.1419600
Subject(s) - pulsar , physics , astrophysics , magnetar , astronomy , neutron star , flux (metallurgy) , x ray pulsar , static timing analysis , glitch , materials science , computer science , metallurgy , embedded system , detector , optics
We report on long-term monitoring of the anomalous X-ray pulsar 1E1048.1-5937 using the Rossi X-ray Timing Explorer. This pulsar's timingbehavior is different from that of other AXPs. In particular, the pulsar showssignificant deviations from simple spin-down such that phase-coherent timinghas not been possible over time spans longer than a few months. We show that inspite of the rotational irregularities, the pulsar exhibits neither pulseprofile changes nor large pulsed flux variations. We discuss the implicationsof our results for AXP models. We suggest that 1E 1048.1-5937 may be atransition object between the soft gamma-ray repeater and AXP populations, andthe AXP most likely to one day undergo an outburst.Comment: 6 pages, to appear in Proceedings of the 20th Texas Symposium on Relativistic Astrophysics, AIP pres
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