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X‐Ray Emission from the Radio‐quiet Neutron Star in Puppis A

  • Authors: V. E. Zavlin, J. Trümper, and G. G. Pavlov

Zavlin, Trümper, & Pavlov 1999 The Astrophysical Journal 525 959.

  • Provider: AAS Journals

Caption: Fig. 4.

68%, 90%, and 99% confidence contours for spectral fits with NS hydrogen atmosphere models (for ﹩M=1.4\,M_{\odot }﹩, ﹩R=10﹩ km, and two values of magnetic field B) to the combined PSPC and GIS2 spectra. The dashed lines in the upper panels delineate the distance range, ﹩d=( 1.9﹩–2.5) kpc, determined from radio observations. The dashed lines in the lower panels show best‐fit ﹩n_{\mathrm{H}\,}﹩ and ﹩T_{\mathrm{eff}\,}﹩ for the upper and lower distance limits.

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