加载中…
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 mas yr, implying a transverse velocity of km s. We derive an age of the pulsar and S147 of only kyr which is a factor of 20 times less than the pulsar’s characteristic age of $\tau_c = 620P_0=139$ 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.

生成讲解博客的中文版本

生成AI智能校验的中文版本