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No Pulsar Wind Nebula in the Southern Blowout Region of the Cygnus Loop

  • Authors: J. P. Halpern, and E. V. Gotthelf

2019 The Astrophysical Journal 882 155.

  • Provider: AAS Journals

Caption: Figure 3.

R-band optical image of the diffuse X-ray source 3XMM J204914.4+290324 obtained on the Hiltner telescope. The field displayed is 3′ × 3′. The 45″ radius circle encompasses most of the X-ray emission. At the center is the galaxy 2MASX J20491447+2903237, the dominant galaxy of a cluster whose fainter members can also be seen in this image.

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