Figure 2 from Probing the Innermost Ejecta Layers in Supernova Remnant Kes 75: Implications for the Supernova Progenitor

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Probing the Innermost Ejecta Layers in Supernova Remnant Kes 75: Implications for the Supernova Progenitor

Authors: Tea Temim, Patrick Slane, Tuguldur Sukhbold, Bon-Chul Koo, John C. Raymond, and Joseph D. Gelfand

2019 The Astrophysical Journal Letters 878 L19.

Provider: AAS Journals

Caption: Figure 2.

Herschel PACS images of the PWN region in Kes 75 at 70, 100, and 160 μm. The white contours represent the Chandra X-ray emission from the PWN. The corresponding measured flux densities are listed in Table 1.

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