Author/Authors :
K. Torii، نويسنده , , K. Kinugasa، نويسنده , , T. Asanuma، نويسنده , , T. Toneri، نويسنده , , H. Tsunemi، نويسنده , , T. Dotani، نويسنده , , K. Mitsuda، نويسنده , , E.V. Gotthelf، نويسنده , , R. Petre، نويسنده ,
Abstract :
During the course of our X-ray studies of composite supernova remnants, we have discovered two young pulsars. The 65 ms pulsar, AX J1811.5-1926, is found to be associated with the central X-ray emission from the candidate of the historical SNR G11.2-0.3; and the 69 ms pulsar near the SNR RCW 103 is identified with a previously reported GINGA pulsator. Here, we present an observational summary of these two pulsars.
