OLD ISOLATED ACCRETING NEUTRON STARS: CONTRIBUTION TO THE SOFT X--RAY BACKGROUND IN THE 0.5--2 KEV BAND

Abstract

The issue of the observability of Old Isolated Neutron Stars (ONSs) accreting from the interstellar gas, is reconsidered using the spectra presented in Zampieri {\it et al.\/} (1995). In particular, we focus our attention on the overall soft X--ray emission of ONSs, which may provide a substantial contribution to the X--ray background in the 0.5--2 keV band. It is found that if accretion is channeled into polar caps by a magnetic field of $\sim 10^9$ G, up to $\sim$ $12-25\%$ of the unresolved soft excess observed at high latitudes in the X--ray background can be explained in terms of emission from accreting isolated ONSs. However, this would imply the detection with ROSAT of $\sim 10$ sources deg${}^{-2}$ above a threshold of $\sim 10^{-14}\mathrm{erg}\mathrm{c}{\mathrm{m}}^{-2}{\mathrm{s}}^{-1}$. A brief reconsideration of the observability of isolated ONSs as individual X--ray sources is also presented.

23 pages plus 5 tables, included at the end as separate TeX files (2 postscript figures available upon request), PlainTeX, submitted to ApJ.

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