B 0628 - 28
نویسندگان
چکیده
PSR B0628-28 is a radio pulsar which was first detected in the X-ray band by ROSAT and then later observed with Chandra and XMM-Newton. The Chan-dra observation yielded an X-ray luminosity two orders of magnitude higher than what is expected for spin-powered pulsars, also there were no pulsations detected. The XMM-Newton observation, however, reveals pulsations at the expected radio period, P = 1.244 s. The simultaneously analyzed spectra also give a luminos-ity (in cgs) log L x = 30.34, which is ∼ 350 times greater than what would be expected from the correlation between L x-˙ E.
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