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 Letters878L19.
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.