A Systematic Study of Quiescent and Outburst Properties of X-ray-bright Young Stellar Objects Using XMM-Newton

arXiv:2607.25384 · astro-ph.SR · Submitted 2026-07-28 · Read on arXiv

Koki Sakuta, Ikuyuki Mitsuishi, Seiya Sasamata, Daigo Nonaka, Mai Yamashita, Shin Toriumi, Takato Tokuno, Yohko Tsuboi, Hiroshi Kobayashi

astro-ph.SR

Submitted: 2026-07-28

Comments: Accepted for publication in Astronomy & Astrophysics. 15 pages, 4 figures, 5 tables

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

Terminology

• Abundance — 12× in this paper · explained in 1 episode
• Accretion Shock — 2× in this paper · explained in 1 episode
• Active Regions — 1× in this paper · explained in 1 episode
• Consistency — 1× in this paper · explained in 3 episodes
• Milky Way Star Clusters — 1× in this paper
• Trace — 1× in this paper · explained in 2 episodes

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