Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-06-30
Astrophys.J.593:L31-L34,2003
Astronomy and Astrophysics
Astrophysics
accepted for publication in ApJ Letters, 13 pages, 3 figures
Scientific paper
10.1086/378082
We present results of timing observations of the 143-ms pulsar J0538+2817 that provide a proper motion measurement which clearly associates the pulsar with the supernova remnant S147. We measure a proper motion of 67$_{-22}^{+48}$ mas yr$^{-1}$, implying a transverse velocity of $v= 385^{+260}_{-130}$ km s$^{-1}$. We derive an age of the pulsar and S147 of only $30\pm4$ kyr which is a factor of 20 times less than the pulsar's characteristic age of $\tau_c = 620$ kyr. This age implies an initial spin period of $P_0=139$ ms, close to the present pulse period and a factor of several larger than what is usually inferred for birth periods. Implications for recent X-ray detections of this pulsar are discussed.
Carr Paul
Hobbs George
Jordan Cathy
Kramer Mallie Mae
Lohmer O.
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