X-NAVI:ET - PSR 0950+08 (X-Ray Emission)


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  1. PSR +08 (X-Ray Emission) Video Tracks: 7: Electric Uranus - Start (Mercury-Atlas 7) 8: X-NAVI:ET - PSR +08 (X-Ray Emission) Notes Electric Uranus (Wojciech Zięba) - Tracks 1, 3, 5 X-NAVI:ET (Rafał Iwański) Tracks 2, 4, 6 Other Versions (1 of 1) /5(8).
  2. Jun 01,  · Marginal evidence of pulsed X-ray emission from PSR +08 is present with % significance and pulsed fraction +/- Relativistic ray tracing shows that if the geometry deduced from the polarization of the radio pulse is adopted for the surface thermal emission, a centered dipole cannot reproduce the large pulse modulations observed unless the radius of the neutron star is as Cited by:
  3. This article presents indirect evidence that on July 29, 19+ 08 emitted a burst of X-ray emissions along with the enhanced radio pulses.
  4. Feb 01,  · The most likely explanation for the emission is that PSR + 08 is surrounded by a synchrotron nebula, which is unresolved and has a spectral index of about 1. For either model the X-ray luminosity ( keV) is about 10 exp 29 erg/hardfounpachanseri.forludeneburbarsciherceticonce.co by:
  5. The most likely explanation for the emission is that PSR + 08 is surrounded by a synchrotron nebula, which is unresolved and has a spectral index of about 1.
  6. Subject headings: pulsars: individual (Geminga, PSR {52, PSR +14, PSR +10, PSR +08) | stars: neutron | X-rays: stars 1. Introduction X-ray emission at keV energies from pulsars may come from several sources: (a) thermal cooling from the entire stellar surface of deep internal heating source (e.g., residual.
  7. Marginal evidence of pulsed X-ray emission from PSR +08 is present with % significance and pulsed fraction +/- Relativistic ray tracing shows that if the geometry deduced from the polarization of the radio pulse is adopted for the surface thermal emission, a central dipole cannot reproduce the large pulsed modulations observed unless the radius of the neutron star is as large as .
  8. The models are compared to X-ray data from Geminga, PSR , PSR +14, PSR +10, and PSR + A model is proposed for the observed combination of power-law and thermal emission of keV X-rays from rotationally powered pulsars.
  9. The models are compared to X-ray data from Geminga, PSR , PSR +14, PSR +10, and PSR + A model is proposed for the observed combination of power-law and thermal emission of keV X-rays from rotationally powered pulsars. For γ-ray pulsars with accelerators very many stellar radii above the neutron star surface, MeV.

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