Image Details

Choose export citation format:

Large resolution
Export to PDF PPT Format

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. 6.

Confidence contours (68% and 90%) for the PL fit to the compact PWN and extended PWN for fixed ﹩n_{\mathrm{H}\,,22}=1.0﹩. The PL normalization is in units of 10−5 photons cm−2 s−1 keV−1 at 1 keV. The dashed curves are the loci of constant unabsorbed flux in the 0.5–8 keV band; the flux values near the curves are in units of 10−13 ergs cm−2 s−1.

Other Images in This Article
Copyright and Terms & Conditions