Comparisons of Different Fitting Methods for the Physical Parameters of a Star Cluster Sample of M33 with Spectroscopy and Photometry
Author:
Funder
National Natural Science Foundation of China
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4365/abb700/pdf
Reference73 articles.
1. Evidence for temporal evolution in the M33 disc as traced by its star clusters
2. A POSSIBLE PHYSICAL CONNECTION BETWEEN HELIUM-RICH STELLAR POPULATIONS OF MASSIVE GLOBULAR CLUSTERS AND THE UV UPTURN OF GALACTIC SPHEROIDS
3. K-Corrections and Filter Transformations in the Ultraviolet, Optical, and Near-Infrared
4. Stellar population synthesis at the resolution of 2003
5. STELLAR LIFETIME AND ULTRAVIOLET PROPERTIES OF THE OLD METAL-RICH GALACTIC OPEN CLUSTER NGC 6791: A PATHWAY TO UNDERSTAND THE ULTRAVIOLET UPTURN OF ELLIPTICAL GALAXIES
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2. Investigating the UV-excess in Star Clusters with N-body Simulations: Predictions for Future CSST Observations*;Research in Astronomy and Astrophysics;2022-08-30
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