RXTE Observations of PSR J1105-6107

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dc.creatorSteinberger, Julia K.
dc.creatorKaspi, Victoria M.
dc.creatorGotthelf, Eric V.
dc.date1998-09-28
dc.date.accessioned2026-07-07T02:28:06Z
dc.date.available2026-07-07T02:28:06Z
dc.descriptionWe report on X-ray observations of the young, energetic radio pulsar PSR J1105-6107 obtained using the Rossi X-ray Timing Explorer. Our timing analysis of Proportional Counter Array data finds no evidence for X-ray pulsations from this source. We set a new upper limit on the pulsed X-ray flux from the pulsar of 18% in the 2-10 keV band, for a duty cycle of 0.5. Our improved upper limit supports the hypothesis that the X-ray emission seen by the ASCA X-ray satellite in the direction of PSR J1105-6107 is the result of a pulsar-powered synchrotron nebula.
dc.identifierhttps://arxiv.org/abs/astro-ph/9809367
dc.identifierhttp://arxiv.org/abs/astro-ph/9809367
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12977
dc.subjectAstrophysics
dc.titleRXTE Observations of PSR J1105-6107
dc.typetext

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