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

Comments: 23 pages, 15 figures, This paper is accepted for publication in RAA

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

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

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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