Proper motion, age and initial spin period of PSR J0538+2817 in S147
Abstract
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 304 kyr which is a factor of 20 times less than the pulsar's characteristic age of τc = 620 kyr. This age implies an initial spin period of P0=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.
Turn this paper into a full lesson
ArcXiv compiles a staged curriculum from this paper: 8-12 lessons across beginner → advanced, synthesised section guides, visuals, flashcards, a quiz, exercises, and on-demand deep dives per section. Grounded in the abstract, never invented.