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20232026
most citedUnveiling the Binary Nature of NGC 2323

7 citations · 11 across the 10 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

Evolution of Compact Stellar Systems in Ultralight Dark Matter Halos: Dependence on Stellar and Dark Matter Parameters

Yu-Ming Yang, Xiao-Jun Bi, Long Wang +1

Compact stellar systems are often used to place stringent constraints on the particle mass of ultralight dark matter (ULDM), as the heating effect induced by wave interference can…

astro-ph.GA2026

Evolution of the stellar mass function in open clusters from a universal and unsegregated initial state

Lu Li, Zhaozhou Li, Zhengyi Shao +2

The stellar mass function (MF) and its spatial variation (mass segregation) within star clusters encode signatures of early formation physics and subsequent secular evolution. Yet,…

astro-ph.GA2026

Binary disruption during the early phase of open clusters

Zepeng Zheng, Long Wang, Holger Baumgardt

The binary fraction in young open clusters exceeds that of field stars, making the study of binary dynamical evolution in clusters essential for understanding the origins and evolu…

astro-ph.GA2025

Cosmic Threads: Interlinking the Stellar Initial Mass Function from Star-Birth to Galaxies

Tereza Jerabkova, Donatella Romano, Pavel Kroupa +19

The stellar initial mass function (sIMF) describes the distribution of stellar masses formed in a single star formation event in a molecular cloud clump. It is fundamental to astro…

astro-ph.GA20247 cited

Unveiling the Binary Nature of NGC 2323

Songmei Qin, Jing Zhong, Tong Tang +9

As a well-known open cluster, NGC 2323 (also called M50) has been widely investigated for over a hundred years and has always been considered a classical single cluster. In this wo…

astro-ph.GA2023

Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars

Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +11

The mode of star formation that results in the formation of globular clusters and young massive clusters is difficult to constrain through observations. We present models of massiv…