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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 5.

Single-temperature dust models fitted to the Herschel PACS SED of the emission associated with the PWN in Kes 75 (flux densities in Table 1). The solid and dotted lines represent the best-fit models for silicate (Weingartner & Draine 2001) and amorphous carbon (Rouleau & Martin 1991) grain compositions, respectively. The corresponding best-fit dust temperatures and masses are listed in Table 3.

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