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Asteroseismology of 3642 Kepler Red Giants: Correcting the Scaling Relations Based on Detailed Modeling
Tanda 坦达 Li 李, Yaguang 亚光 Li 李, Shaolan 少兰 Bi 毕, Timothy R. Bedding, Guy Davies and Minghao 明昊 Du 杜 The Astrophysical Journal 927(2) 167 (2022) https://doi.org/10.3847/1538-4357/ac4fbf
Age dissection of the Milky Way discs: Red giants in theKeplerfield
New parsec data base of α-enhanced stellar evolutionary tracks and isochrones – I. Calibration with 47 Tuc (NGC 104) and the improvement on RGB bump
Xiaoting Fu, Alessandro Bressan, Paola Marigo, et al. Monthly Notices of the Royal Astronomical Society 476(1) 496 (2018) https://doi.org/10.1093/mnras/sty235
Diagnostics of stellar modelling from spectroscopy and photometry of globular clusters
George C. Angelou, Valentina D'Orazi, Thomas N. Constantino, et al. Monthly Notices of the Royal Astronomical Society 450(3) 2423 (2015) https://doi.org/10.1093/mnras/stv770
ISOCHRONES FOR OLD (>5 GYR) STARS AND STELLAR POPULATIONS. I. MODELS FOR –2.4 ⩽ [Fe/H] ⩽+0.6, 0.25 ⩽Y⩽ 0.33, AND –0.4 ⩽ [α/Fe] ⩽+0.4
Red Giants as Probes of the Structure and Evolution of the Milky Way
Maurizio Salaris Astrophysics and Space Science Proceedings, Red Giants as Probes of the Structure and Evolution of the Milky Way 45 (2012) https://doi.org/10.1007/978-3-642-18418-5_5
Giants reveal what dwarfs conceal: Li abundance in lower red giant branch stars as diagnostic of the primordial Li★
Corinne Charbonnel, Marco Limongi, Francesca D'Antona, et al. Proceedings of the International Astronomical Union 7(T28A) 161 (2011) https://doi.org/10.1017/S1743921312002773
The magnitude difference between the main sequence turn off and the red giant branch bump in Galactic globular clusters