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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 10.

The curves represent the elemental mass ratios (after the subtraction of the NS mass) as a function of the ZAMS mass, based on the CC models of Jacovich et al. (2021; solid lines) and Sukhbold et al. (2016; dotted lines). We note that since these models overpredict the Mg and underpredict the Ne masses (see Section 4.1), the Mg/O curve would move down and the Ne/O curve would move up, as indicated by the colored arrows. The colored bands represent the elemental mass ratios as measured from X-ray observations by Bhalerao et al. (2019). A ZAMS mass of around 13 M gives abundance ratios that are roughly consistent with the total oxygen mass in the last panel and the measured ratios of Fe, Si, and S with respect to oxygen.

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