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Titlebook: Not-So-Simple Stellar Populations in Star Clusters; Chengyuan Li Book 2017 Springer Nature Singapore Pte Ltd. 2017 Progenitor molecular cl

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樓主: 貶損
21#
發(fā)表于 2025-3-25 03:42:53 | 只看該作者
Researches of Stellar Populations in Star Clusterss of SSPs for a long time until the discoveries of MSPs in GCs, which have expanded our view on stellar populations in SCs. This chapter introduces our traditional thought on stellar populations in SCs, the history and progress of researches in this active field were also present.
22#
發(fā)表于 2025-3-25 10:51:40 | 只看該作者
23#
發(fā)表于 2025-3-25 15:02:27 | 只看該作者
The Formation and Evolution of Blue Straggler Stars in Globular Cluster binaries in a SC. However, the hard binaries would survive at this stage and continue with their further evolution, which would finally lead them to merge, resulting in BSS. Especially for binaries that contain massive stars, only a small fraction of them would evolve undisturbed towards their supe
24#
發(fā)表于 2025-3-25 17:20:26 | 只看該作者
Multiple Stellar Populations in the Giant Branches of Galactic Globular ClustersB and RGB in its CMD, the morphology of its giant branches is consistent with the description in Sect.?., which can be ideally described as a combination of stellar populations with different ages, helium abundances and metallicities. The broadening in its giant branches is spatially dependent, with
25#
發(fā)表于 2025-3-25 22:04:18 | 只看該作者
26#
發(fā)表于 2025-3-26 01:58:01 | 只看該作者
27#
發(fā)表于 2025-3-26 06:38:41 | 只看該作者
28#
發(fā)表于 2025-3-26 11:50:56 | 只看該作者
29#
發(fā)表于 2025-3-26 15:19:30 | 只看該作者
2190-5053 h introduced in this book reveals key features of star clusters formation and by extension how all stars formed in our universe..978-981-13-5461-8978-981-10-5681-9Series ISSN 2190-5053 Series E-ISSN 2190-5061
30#
發(fā)表于 2025-3-26 16:52:20 | 只看該作者
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