Light curve spectral energy distribution fitting of 13 carbon-rich Mira variables stars in the Small Magellanic Cloud

arXiv:2610.09537 · astro-ph.SR, astro-ph.GA · Submitted 2026-10-07 · Read on arXiv

astro-ph.SR, astro-ph.GA

Submitted: 2026-10-07

Updated: 2026-10-07

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