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astro-ph.GA2025
Tides from the cloud can induce the fast disruption of star clusters and offer an explanation for Gaia strings
Xiao-Tong Chen, Guang-Xing Li
Young stars form in clusters within molecular clouds, but older stars are evenly distributed across the galactic disk, necessitating an explanation for cluster dissolution. We anal…
astro-ph.GA2025
Kinematics of the interstellar medium using Gaia: A catalogue of 102 YSO-MC associations within 3.5 kpc from the Sun with 3D velocities
Ji-Xuan Zhou, Guang-Xing Li, Bing-Qiu Chen
Kinematic information is crucial for understanding the evolution of complex systems, such as interstellar gas. Obtaining full 3D kinematic information is a crucial final step for m…
astro-ph.GA2025★ 3 cited
Shear-gravity transition determines the steep velocity dispersion-size relation in molecular clouds: confronting analytical formula with observations
Yi-Heng Xie, Guang-Xing Li
The velocity dispersion-size relation () is a crucial indicator of the dynamic properties of interstellar gas, where the slope is considered as . Rece…