Post-Glitch RXTE-PCA Observations of the Vela Pulsar
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We report the results of analysis of observations of the Vela Pulsar by PCA on RXTE. Our data consists of two parts. The first part contains observations at 1, 4, and 9 days after the glitch in 1996 and has 27000 sec. total exposure time. The second part of observations were performed three months after this glitch and have a total exposure time of 93000 sec. We found pulsations in both sets. The observed spectrum is a power-law with no apparent change in flux or count rate. The theoretical expectations of increase in flux due to internal heating after a glitch are smaller than the uncertainty of the observations.
6 pages, 5 figures in 9 ps/eps files. Accepted for publication in A&A Main Journal
6 pages, 5 figures in 9 ps/eps files. Accepted for publication in A&A Main Journal