Oxygen Isotopic Compositions of Chondrules as Probes of Solar Protoplanetary Disk Formation

arXiv:2604.25263 · astro-ph.EP, astro-ph.SR · Submitted 2026-04-28 · Read on arXiv

astro-ph.EP, astro-ph.SR

Submitted: 2026-04-28

Updated: 2026-04-28

DOI: 10.3847/1538-4357/ae93a1

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 98× in this paper · explained in 2 episodes
• Abundance — 16× in this paper · explained in 1 episode
• Primitive Chondrule Materials — 2× in this paper
• Accretion Flows — 1× in this paper · explained in 1 episode
• Angular Momentum Transport — 1× in this paper · explained in 3 episodes
• Phase Transitions — 1× in this paper · explained in 2 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• From Bubbles and Filaments to Cores and Disks: Gas Gathering and Growth of Structure Leading to the Formation of Stellar Systems
• The role of magnetic fields in the formation of protostars, disks, and outflows

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