HEAD 2000, November 2000
Session 32. Supernova Remnants/ISM
Display, Thursday, November 9, 2000, 8:00am-6:00pm, Bora Bora Ballroom

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[32.16] A Search for Pulsed Emission from Kepler using RXTE

G.E. Allen (MIT CSR), A. Decourchelle (CEA Saclay)

We present an analysis of RXTE timing data of the Kepler supernova remnant. Power density spectral results will be presented for a broad energy range and separately for low, medium, and high-energy X-ray bands. The pulsed-flux limits will be presented. This work is supported in part by contract SAO SV1-61010.

The author(s) of this abstract have provided an email address for comments about the abstract: gea@space.mit.edu

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