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- W3100972754 abstract "Context. It is believed that some other parameters, except for metallicity (the first parameter), are needed to explain the horizontal branch (HB) morphology of globular clusters (GCs). Furthermore, these parameters are considered to be correlated with the mass loss of the red giant branch (RGB) stars. Unfortunately, the physics of mass loss on the RGB is poorly understood at present. In our previous work, we proposed that tidally enhanced stellar wind during binary evolution may affect the HB morphology by enhancing the mass loss of the red giant primary and that we can reproduce the basic morphology of HB in GCs." @default.
- W3100972754 created "2020-11-23" @default.
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- W3100972754 date "2013-06-01" @default.
- W3100972754 modified "2023-10-16" @default.
- W3100972754 title "Synthetic horizontal branch morphology for different metallicities and ages under tidally enhanced stellar wind" @default.
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- W3100972754 doi "https://doi.org/10.1051/0004-6361/201220998" @default.
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