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An ASCA Observation of M51 (NGC 5194): Iron K Emission from an Obscured Active Galactic Nucleus

  • Authors: Y. Terashima, A. Ptak, R. Fujimoto, M. Itoh, H. Kunieda, K. Makishima, and P. J. Serlemitsos

Terashima et al. 1998 The Astrophysical Journal 496 210.

  • Provider: AAS Journals

Caption: Fig. 1.

Contour map of M51 and NGC 5195 taken with SIS detectors (SIS0 + SIS1) superposed on optical image. Background is not subtracted. The contour levels are logarithmically spaced. The region between dashed lines is used to make a projected brightness profile presented in Fig. 2.

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