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Titlebook: Isolated Neutron Stars: From the Surface to the Interior; Silvia Zane,Roberto Turolla,Dany Page Conference proceedings 2007 Springer Scien

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31#
發(fā)表于 2025-3-26 21:19:46 | 只看該作者
32#
發(fā)表于 2025-3-27 03:28:42 | 只看該作者
33#
發(fā)表于 2025-3-27 09:03:06 | 只看該作者
in April 2006. Forty years after the discovery of radio pulsars it presents an up-to-date description of the new vision of isolated neutron stars that has emerged in recent years with the advance of multi-wavelength observations. The great variety of isolated neutron stars, from pulsars to magnetar
34#
發(fā)表于 2025-3-27 10:49:34 | 只看該作者
Conference proceedings 20072006. Forty years after the discovery of radio pulsars it presents an up-to-date description of the new vision of isolated neutron stars that has emerged in recent years with the advance of multi-wavelength observations. The great variety of isolated neutron stars, from pulsars to magnetars, some of
35#
發(fā)表于 2025-3-27 13:36:18 | 只看該作者
36#
發(fā)表于 2025-3-27 21:06:29 | 只看該作者
Our distorted view of magnetars: application of the resonant cyclotron scattering model,e neutron star surface, resulting in production of non-thermal spectra. Here we discuss the Resonant Cyclotron Scattering (RCS) model, and present its XSPEC implementation, as well as preliminary results of its application to Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters.
37#
發(fā)表于 2025-3-27 23:32:37 | 只看該作者
Chandra smells a RRAT,itous detection with the . of a bright point-like X-ray source coincident with one of the RRATs. We discuss the temporal and spectral properties of this X-ray emission, consider counterparts in other wavebands, and interpret these results in the context of possible explanations for the RRAT population.
38#
發(fā)表于 2025-3-28 03:16:28 | 只看該作者
39#
發(fā)表于 2025-3-28 09:44:24 | 只看該作者
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發(fā)表于 2025-3-28 12:37:28 | 只看該作者
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