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The Magnificent Seven: Close-by Cooling Neutron Stars? | A. Treves
; S.B. Popov
; M. Colpi
; M.E. Prokhorov
; R. Turolla
; | Date: |
30 Nov 2000 | Subject: | astro-ph | Affiliation: | Univ. of Como), S.B. Popov (SAI), M. Colpi (Univ. of Milan), M.E. Prokhorov (SAI) and R. Turolla (Univ. of Padova | Abstract: | We model Galactic populations of accreting and cooling isolated neutron stars in the attempt to explore their link with a new class of dim soft X-ray sources revealed by ROSAT. For accretors we follow the magneto-rotational and dynamical evolution in the Galactic potential and a realistic large scale distribution of the interstellar medium is used. Under standard assumptions old neutron stars enter the accretor stage only if their magnetic field exceeds $approx 10^{11}$--$10^{12}$ G. We predict about 1 source per square degree for fluxes $approx 10^{-15}$--$10^{-16}$ erg cm$^{-2}$s$^{-1}$ in the energy range 0.5-2 keV. Cooling neutron stars are explored within a simpler model of local sources, including however interstellar absorption. They are found to be significantly less abundant at low fluxes, $<0.1$ sources per square degree, but dominate over accretors at higher flux levels ($approx 10^{-12}$--$10^{-11}$ erg cm$^{-2}$s$^{-1}$). We suggest that the faint sources observed by ROSAT may be young cooling neutron stars with typical age $la 10^6$ yrs, if the total number of young neutron stars in the Solar proximity is $sim 10$ times higher than inferred from radiopulsars statistics. | Source: | arXiv, astro-ph/0011564 | Services: | Forum | Review | PDF | Favorites |
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