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SNR G292.0+1.8: A Remnant of a Low-mass-progenitor Stripped-envelope Supernova

  • Authors: Tea Temim, Patrick Slane, John C. Raymond, Daniel Patnaude, Emily Murray, Parviz Ghavamian, Mathieu Renzo, Taylor Jacovich

Tea Temim et al 2022 The Astrophysical Journal 932 .

  • Provider: AAS Journals

Caption: Figure 8.

The total ejecta mass (black curve), He core mass (dark gray curve), and CO core mass (light gray curve) as a function of the ZAMS mass for the single-star CC models of Jacovich et al. (2021). The green curve represents the total mass of O, Ne, Mg, Si, S, and Fe inside the He core as a function of the ZAMS mass. All curves exclude the NS mass. The horizontal green band indicates the total X-ray-measured mass of O, Ne, Mg, Si, S, and Fe, including the uncertainties (Bhalerao et al. 2019). The gray vertical band marks the corresponding range of consistent ZAMS masses.

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