摘要： We report recent XMM-Newton investigations of PSR J1836+5925, the "next Geminga," which determined an X-ray pulsation of ~ 173.3 ms. Its X-ray periodicity is consistent with the y-ray ephemeris at the same epoch. The X-ray folded light curve has a sinusoidal structure that is different from the double-peaked y-ray pulse profile. We have also analyzed the X-ray phase-averaged spectra which shows that the X-ray emission from PSR J1836+5925 is thermal dominant. This suggests that the X-ray pulsation mainly originates from the modulated hot spot on the stellar surface. 出版者： United States 出版日期： 2014-09-20 出處： Astrophysical journal. Letters, 2014-09, Vol.793 (1), p.L8-4 資源來源： Institute of Physics Journals 識別號： ISSN: 2041-8213 識別號： ISSN: 2041-8205 識別號： EISSN: 2041-8213 識別號： DOI: 10.1088/2041-8205/793/1/L8
