A formation pathway for giant planets in S-type discs of gamma-Cephei-like compact binaries

arXiv:2605.05085 · astro-ph.EP · Submitted 2026-05-06 · Read on arXiv

María Paula Ronco, Octavio M. Guilera, Julia Venturini, Federico Zoppetti, Marcelo M. Miller Bertolami

astro-ph.EP

Submitted: 2026-05-06

Comments: Accepted for publication in A&A - 16 pages, 10 figures

Code: https://github.com/Aryy98/Circumstellar_disc_truncation_radius

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

Terminology

• Core — 14× in this paper · explained in 2 episodes
• Accretion Efficiency — 2× in this paper · explained in 2 episodes
• Metallicity — 2× in this paper · explained in 3 episodes
• Abundance — 1× in this paper · explained in 1 episode
• Alignment — 1× in this paper · explained in 1 episode
• N-body simulations — 1× in this paper · explained in 2 episodes
• Streaming Instability — 1× in this paper · explained in 2 episodes

Sources

• Giant planet formation at the pressure maxima of protoplanetary disks II. A hybrid accretion scenario

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