Small-scale structure deduced from X- and gamma-ray timing measurements

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dc.creatorMiller, M. Coleman
dc.date2000-12-02
dc.date.accessioned2026-07-07T01:56:49Z
dc.date.available2026-07-07T01:56:49Z
dc.descriptionX-ray timing observations of neutron stars and black holes are among the few available probes of ultrastrong magnetic fields, strong gravity, high densities, and the propagation of thermonuclear burning. Here we review the evidence for these effects revealed with data from the Rossi Explorer in the last five years. We also discuss the exciting prospects for making the first quantitative tests of strong-gravity general relativistic predictions with a large-area X-ray timing mission.
dc.description8 pages including 2 figures, uses newpasp.sty (included), invited talk at IAU Symposium #205
dc.identifierhttps://arxiv.org/abs/astro-ph/0012043
dc.identifierhttp://arxiv.org/abs/astro-ph/0012043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2140
dc.subjectAstrophysics
dc.titleSmall-scale structure deduced from X- and gamma-ray timing measurements
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