Chemical complexity in feedback from supernova remnants: first detection of PO+ in IC443 and W44

arXiv:2610.01211 · astro-ph.GA, astro-ph.HE, astro-ph.SR · Submitted 2026-10-01 · Read on arXiv

astro-ph.GA, astro-ph.HE, astro-ph.SR

Submitted: 2026-10-01

Updated: 2026-10-01

Terminology

• Abundance — 57× in this paper · explained in 1 episode
• Core — 9× in this paper · explained in 2 episodes
• Aperture — 4× in this paper · explained in 1 episode
• Trace — 3× in this paper · explained in 2 episodes

Related papers

• Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
• Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
• Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
• Deriving volume density profiles of filaments from observed surface densities
• Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
• MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies