Other
Scientific paper
Aug 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004head....8.0820t&link_type=abstract
American Astronomical Society, HEAD meeting #8, #08.20; Bulletin of the American Astronomical Society, Vol. 36, p.920
Other
Scientific paper
On June 18 2002, the Anomalous X-ray Pulsar AXP 1E 2259+586 underwent a major X-ray outburst that lasted several hours and consequently linked AXP's to another class of high-energy bursting objects, called Soft Gamma-ray Repeaters (SGR). This was predicted uniquely by the "magnetar" model, in which these two classes are ultrahigh magnetic field, isolated young neutron stars. A few days after this outburst, Target of Opportunity observations were obtained with the Gemini North Near-InfraRed Imager (NIRI), followed by a longer term monitoring program of the IR variability that spanned nearly one and a half years. It was observed that shortly after the burst, the pulsar's Ks band flux dramatically increased relative to its pre-burst flux level, prompting the question "does the IR luminosity of 1E 2259+586 constantly undergo fluctuations, or can this brightening be undeniably associated with the X-ray outburst?" We present the results of our IR analysis, and relate them to the results of previous X-ray studies. There was clear evidence of a correlation between the IR flux decay and that of the long-term X-ray afterglow, implying that the IR enhancement was definitely linked to the outburst. We use this correlation to apply constraints on current AXP theoretical models.
Durant Martin
Kaspi Victoria M.
Tam Cindy R.
van Kerkwijk Marten Henric
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