SPIRITS 19q: Dust Production by a Subsolar-metallicity Carbon-rich Wolf-Rayet Star in NGC 2403

arXiv:2609.00477 · astro-ph.SR, astro-ph.GA · Submitted 2026-08-31 · Read on arXiv

astro-ph.SR, astro-ph.GA

Submitted: 2026-08-31

Updated: 2026-08-31

Terminology

• Metallicity — 22× in this paper · explained in 3 episodes
• Abundance — 3× in this paper · explained in 1 episode
• Aperture — 3× in this paper · explained in 1 episode
• Asymptotic Giant Branch — 2× in this paper
• Calibration — 2× in this paper · explained in 7 episodes
• Adam — 1× in this paper · explained in 2 episodes
• Aperture Photometry — 1× in this paper · explained in 1 episode
• Binary Population and Spectral Synthesis — 1× in this paper
• Boltzmann Equation — 1× in this paper · explained in 2 episodes
• Core — 1× in this paper · explained in 2 episodes
• Keck Observatory Archive — 1× in this paper
• Mikulski Archive for Space Telescopes — 1× in this paper

Sources

• The Large Magellanic Cloud: Structure and Kinematics
• Carbonaceous dust grains seen in the first billion years of cosmic time

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