activity
20132024
most citedCombined Effects of Binaries and Stellar Rotation on the Color-Magnitude Diagrams of Intermediate-Age Star Clusters

44 citations · 150 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2024★ 1 cited

BSEC method for unveiling open clusters and its application to Gaia DR3: 83 new clusters

Zhongmu Li, Caiyan Mao

Open clusters (OCs) are common in the Milky Way, but most of them remain undiscovered. There are numerous techniques (e.g., machine-learning algorithms) available for the explorati…

astro-ph.SR2021

A database of spectral energy distributions of progenitors of core-collapse supernovae

Zhongmu Li, Caiyan Mao

This paper presents a database of the spectroscopic- and photometric- spectral energy distributions (spec-SEDs and phot-SEDs) of the progenitors of core-collapse supernovae (CCSNe)…

astro-ph.GA2017★ 28 cited

Powerful CMD: A Tool for Colour-Magnitude Diagram Studies

Zhong-Mu Li, Cai-Yan Mao, Qi-Ping Luo +5

We present a new tool for colour-magnitude diagram (CMD) studies, . This tool is built on the basis of the advanced stellar population synthesis (ASPS) model, in whic…

astro-ph.SR2016★ 31 cited

A systematic study of effects of stellar rotation, age spread and binaries on color-magnitude diagrams with extended main-sequence turn-offs

Zhongmu Li, Caiyan Mao, Liyun Zhang +2

Stellar rotation, age spread and binary stars are thought to be three most possible causes of the peculiar color-magnitude diagrams (CMDs) of some star clusters, which exhibit exte…

astro-ph.SR2015★ 1 cited

Failure of rotation and notable success of age spread to reproduce the CMDs of star clusters NGC 1831, NGC 1868 and NGC 2249

Zhongmu Li, Caiyan Mao, Liyun Zhang

We study the high-quality CMDs of three star clusters, NGC 1831, NGC 1868 and NGC 2249 in detail, via the two most likely causes (stellar rotation and age spread) for CMDs with ext…

astro-ph.SR2015★ 24 cited

Explanation of a special color-magnitude diagram of star cluster NGC 1651 from different models

Zhongmu Li, Caiyan Mao, Li Chen

The color-magnitude diagram (CMD) of globular cluster NGC1651 has special structures including a broad main sequence, an extended main sequence turn-off and an extended red giant c…