44 citations · 373 across the 32 of their papers we have counts for
32 papers
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)…
The Ages of M31 Star Clusters: Spectral Energy Distribution Versus Color-Magnitude Diagram
Zhou Fan, Zhongmu Li, Gang Zhao
It is well-known that fitting the Color Magnitude Diagrams (CMDs) to the theoretical isochrones is the main method to determine star cluster ages. However, when the CMDs are not av…
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…
Lick Indices and Spectral Energy Distribution Analysis based on an M31 Star Cluster Sample: Comparisons of Methods and Models
Zhou Fan, Richard de Grijs, Bingqiu Chen +3
Application of fitting techniques to obtain physical parameters---such as ages, metallicities, and -element to iron ratios---of stellar populations is an important approach to u…
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…
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…