1 citations · 1 across the 4 of their papers we have counts for
Showing astro-ph.GAShow all
3 papers · 1 filter
astro-ph.GA2026
Investigating the initial conditions of globular clusters via -body simulations: I. half-mass radius and stellar density
Ruoyun Huang, Baitian Tang, Long Wang +5
Born out of the turbulent, dense gas of the early Universe, globular clusters (GCs) represent a significantly different star-formation mode compared to the local Universe. To quant…
astro-ph.GA2026
Tracing the kinematic perturbations of the Milky Way spiral arms with APOGEE DR17 and Gaia DR3
Xi-Can Tang, Zhi Li, Iulia T. Simion +4
Aims. We constrain the dynamical perturbations of the spiral arms in the Milky Way disk, based on the non-axisymmetric streaming motions of RGB stars revealed by APOGEE and \textit…
astro-ph.GA2024
Where do they come from? Identification of globular cluster escaped stars
Cheng Xu, Baitian Tang, Chengyuan Li +5
Globular clusters (GCs), as old as our Galaxy, constantly lose their members to the field as they cross through the Milky Way (MW). These GC escaped stars (or escapees) are suggest…