[Previous] | [Session 32] | [Next]
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