Competitive roles of turbulence and magnetic field on the formation of unipolar outflows in isolated molecular cloud cores

arXiv:2610.26176 · astro-ph.SR, astro-ph.EP, astro-ph.GA · Submitted 2026-10-19 · Read on arXiv

astro-ph.SR, astro-ph.EP, astro-ph.GA

Submitted: 2026-10-19

Updated: 2026-10-19

Comments: Accepted for publication in PASJ

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

Terminology

• Core — 1× in this paper · explained in 2 episodes

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Finite-Element Asteroseismology I: Two-Dimensional Adiabatic Oscillations of Rapidly Rotating N=3 Polytropes
• Constraining the origin of magnetic white dwarfs
• EPRV Asteroseismology of the K dwarfs GJ 570 A and GJ 783 A with ESPRESSO. Empirical mode-amplitude scaling in tension with 3D convection simulations
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting