Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant
XRISM collaboration

TL;DR
This study detects phosphorus, chlorine, and potassium in the Cassiopeia A supernova remnant using high-resolution X-ray spectroscopy, revealing that stellar activity like rotation and binary interactions significantly influence odd-Z element production.
Contribution
First observational detection of P, Cl, and K in Cassiopeia A with high-resolution X-ray spectroscopy, highlighting the importance of stellar activity in nucleosynthesis of odd-Z elements.
Findings
K detected at above 6σ significance
Standard supernova models underestimate Cl and K abundances
Models including stellar rotation and binary interactions match observations
Abstract
The elements in the universe are synthesized primarily in stars and supernovae, where nuclear fusion favors the production of even-Z elements. In contrast, odd-Z elements are less abundant and their yields are highly dependent on detailed stellar physics, making theoretical predictions of their cosmic abundance uncertain. In particular, the origin of odd-Z elements such as phosphorus (P), chlorine (Cl), and potassium (K), which are important for planet formation and life, is poorly understood. While the abundances of these elements in Milky Way stars are close to solar values, supernova explosion models systematically underestimate their production by up to an order of magnitude, indicating that key mechanisms for odd-Z nucleosynthesis are currently missing from theoretical models. Here we report the observation of P, Cl, and K in the supernova remnant Cassiopeia A using high-resolution…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
