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Article overview
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Old Isolated Accreting Neutron Stars: The Diffuse X--ray Emission From The Galactic Center | | Silvia Zane
; Roberto Turolla
; Aldo Treves
; | | Date: |
14 May 1996 | | Abstract: | The contribution of weakly--magnetized ($Bsim 10^9$ G) neutron stars accreting the interstellar medium to the diffuse X--ray emission observed in the Galactic Center is investigated. It is shown that, under rather conservative assumptions about the neutron stars and gas distributions, the accretion luminosity can account for a sizable fraction, possibly most, of the detected X--ray flux in the 2.5--7 keV band. In particular, model results are compared with {it Granat/} data and show a general agreement in both the flux energy and radial distributions. | | Source: | arXiv, astro-ph/9605071 | | Services: | Forum | Review | PDF | Favorites | |
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