A comprehensive multi-wavelength study of two X-ray emitting Be stars

arXiv:2609.28719 · astro-ph.SR, astro-ph.HE · Submitted 2026-09-23 · Read on arXiv

astro-ph.SR, astro-ph.HE

Submitted: 2026-09-23

Updated: 2026-09-23

Code: https://github.com/mpaegert/tic_inspect

Terminology

• Calibration — 4× in this paper · explained in 7 episodes
• Abundance — 3× in this paper · explained in 1 episode
• Consistency — 3× in this paper · explained in 3 episodes
• Analyzer — 2× in this paper · explained in 1 episode
• Aperture — 2× in this paper · explained in 1 episode
• Chandra X-ray Center — 2× in this paper
• Accretion Flows — 1× in this paper · explained in 1 episode
• Nordic Optical Telescope — 1× in this paper
• Society of Photo-Optical Instrumentation Engineers — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes
• Zwicky Transient Facility — 1× in this paper

Sources

• The magnetic fields in Be stars are stronger than previously suggested

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