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- W65488712 abstract "The observed spectra of many thermally emitting neutron stars (The “Magnificent Seven”, High-Field Pulsars, etc.) suggest that the surface temperature distribution can be described by hot polar regions surrounded by a cooler equatorial belt. The hotter polar “caps” produce pulsed fractions (PF ) in the x-ray emission that, in some cases, can be quite high (e.g. PSR J1119-6127 with PF = 74± 14%, [3]). In neutron stars, such a temperature distribution can be explained by the presence of a strong toroidal field in the crust ([1], [2]). An elegant description of the relationship between pulsed fraction and rg/R for compact stars with hot spots was first given by Beloborodov et al. [4]. In this study, the relationship between pulsed fraction and stellar radius (PF vs. R) for various configurations of hot spot position, beaming factor and observer angle for a 1.4 solar mass neutron star is explored. The pertinence of spot temperature and size is also examined." @default.
- W65488712 created "2016-06-24" @default.
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- W65488712 date "2008-01-01" @default.
- W65488712 modified "2023-09-24" @default.
- W65488712 title "Observable pulsed fractions of thermal emission from neutron stars with toroidal magnetic fields." @default.
- W65488712 hasPublicationYear "2008" @default.
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