Fig. 7 from Chandra Observation of PSR B1823−13 and Its Pulsar Wind Nebula

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Chandra Observation of PSR B1823−13 and Its Pulsar Wind Nebula

Authors: G. G. Pavlov, O. Kargaltsev, and W. F. Brisken

Pavlov, Kargaltsev, & Brisken 2008 The Astrophysical Journal 675 683.

Provider: AAS Journals

Caption: Fig. 7.

Confidence contours (68% and 90%) for the PL fit to the pulsars’s spectrum. The PL normalization is in units of 10⁻⁵ photons cm⁻² s⁻¹ keV⁻¹ at 1 keV. The dashed curves are the lines of constant unabsorbed flux in the 0.5–8 keV band (the flux values are in units of 10⁻¹⁴ ergs cm⁻² s⁻¹).

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