Fig. 4 from A New X‐Ray Flare from the Galactic Nucleus Detected with the XMM‐Newton Photon Imaging Cameras

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A New X‐Ray Flare from the Galactic Nucleus Detected with the XMM‐Newton Photon Imaging Cameras

Authors: A. Goldwurm, E. Brion, P. Goldoni, P. Ferrando, F. Daigne, A. Decourchelle, R. S. Warwick, and P. Predehl

Goldwurm et al. 2003 The Astrophysical Journal 584 751.

Provider: AAS Journals

Caption: Fig. 4.

Count spectra from MOS (black data point set) and PN (red data point set) data, extracted from a region of 10^{﹩\arcsec﹩} radius around Sgr A* during the flare after subtraction of the nonflaring spectra. The spectra are compared to the best‐fit model of an absorbed power law without dust scattering (see Table 2).

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