Molecular and Atomic Gas Associated with the Gamma Ray Supernova Remnant RCW 103

arXiv:2608.24187 · astro-ph.HE, astro-ph.GA · Submitted 2026-08-25 · Read on arXiv

astro-ph.HE, astro-ph.GA

Submitted: 2026-08-25

Updated: 2026-08-25

Terminology

• Calibration — 3× in this paper · explained in 7 episodes
• National Astronomical Observatory of Japan — 3× in this paper
• Australia Telescope Compact Array — 2× in this paper
• Core — 2× in this paper · explained in 2 episodes
• National Institutes of Natural Sciences — 2× in this paper
• Atacama Compact Array — 1× in this paper
• Cooperation — 1× in this paper · explained in 2 episodes
• Verification — 1× in this paper · explained in 2 episodes

Sources

• Multi-Scale CLEAN deconvolution of radio synthesis images
• The gamma-ray visibility of supernova remnants: a test of cosmic ray origin
• A retrospective view of Miriad

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