Copertina

Convective Mixing: The Formation Channel of Li-rich Giants

Fuente: arXiv

Salvato in:

Dettagli Bibliografici
Autori principali:	Li, Xuefeng, Shi, Jianrong, Li, Yan, Yan, Hongliang, Zhang, Jinghua
Natura:	Preprint
Pubblicazione:	2024
Soggetti:	Solar and Stellar Astrophysics
Accesso online:	Acceder al recurso
Tags:	Aggiungi Tag Nessun Tag, puoi essere il primo ad aggiungerne!!

Documenti analoghi

Distribution and evolution of Li abundance in red clump stars can be explained by the internal gravity waves
di: Li, Xuefeng, et al.
Pubblicazione: (2024)

Effect of Matter Accretion on Lithium Enhancement of Giants
di: Li, Xuefeng, et al.
Pubblicazione: (2025)

Meridional Circulation II: A Unified Mechanism for Lithium Depletion in Solar Analogs and the Lithium Dip in Mid-F Cluster Stars
di: Li, Xuefeng, et al.
Pubblicazione: (2025)

Meridional Circulation. I. A Formation Channel for Lithium-rich and Super Lithium-rich Red Clump Stars
di: Li, Xue-Feng, et al.
Pubblicazione: (2025)

Identify ~20,000 Li-rich Giants in the LAMOST Low-Resolution Survey
di: Ding, Ming-Yi, et al.
Pubblicazione: (2026)

Unevolved Li-rich stars at low metallicity: a possible formation pathway through novae
di: Matsuno, Tadafumi, et al.
Pubblicazione: (2025)

The temporal and spatial variations of lithium abundance in the Galactic disc
di: Sun, Tiancheng, et al.
Pubblicazione: (2024)

Discovery of an Extremely Luminous Type II Cepheid in the Andromeda Giant Stellar Stream: Evidence for a Hierarchical Triple with an Inner Binary Merger
di: Chen, Pinjian, et al.
Pubblicazione: (2026)

Probing Red Giant Interiors with G-Dominated Mixed Modes I: The Cases of KIC 9145955, KIC 9970396, KIC 9882316 and KIC 11968334
di: Zhang, Xinyi, et al.
Pubblicazione: (2026)

The transport of angular momentum for massive stars I. Formation of slowly rotating WNE stars
di: Si, Jijuan, et al.
Pubblicazione: (2025)

Formation of WNL stars for the MW and LMC based on the k-omega model
di: Si, Jijuan, et al.
Pubblicazione: (2024)

Potential Impact of the Sagittarius Dwarf Galaxy on the Formation of Young O-rich Stars
di: Sun, Tiancheng, et al.
Pubblicazione: (2023)

PhDLspec: physical-prior embedded deep learning method for spectroscopic determination of stellar labels in high-dimensional parameter space
di: Wu, Tianmin, et al.
Pubblicazione: (2026)

Formation of Giant Planets
di: Youdin, Andrew N., et al.
Pubblicazione: (2025)

The Impact of Initial Mass Dependent Convective Boundary Mixing on the Structure and Fates of Massive Stars
di: Whitehead, Emily E., et al.
Pubblicazione: (2025)

Stellar atmospheric parameters of $\sim$ 11,000 RR Lyrae stars from LAMOST Spectra
di: Wang, Jiangtao, et al.
Pubblicazione: (2024)

Properties of Carbon-rich Asymptotic Giant Branch Stars in the LMC and the Milky Way
di: Suh, Kyung-Won
Pubblicazione: (2025)

Realistic Uncertainties for Fundamental Properties of Asteroseismic Red Giants and the Interplay Between Mixing Length, Metallicity and $ν_{\rm max}$
di: Li, Yaguang, et al.
Pubblicazione: (2024)

Technetium-rich M Stars: Prime diagnostics of recent third dredge-up events on the Asymptotic Giant Branch
di: Shetye, Shreeya, et al.
Pubblicazione: (2025)

A Study of Subsurface Convection Zones of Fast Rotating Massive Stars
di: He, Xiao-long, et al.
Pubblicazione: (2025)

A Panchromatic JWST Spectrum of a Giant Starspot on the Fully Convective M-dwarf TOI-3884
di: Murray, C. A., et al.
Pubblicazione: (2026)

Prediction of Large Solar Flares Based on SHARP and HED Magnetic Field Parameters
di: Li, Xuebao, et al.
Pubblicazione: (2024)

Calibrating the Color-Magnitude Relation of M Giants by Using Open Clusters
di: Tang, Xiaoyu, et al.
Pubblicazione: (2025)

Phase II of the LAMOST-Kepler/K2 Survey. II. Time Domain of Medium-resolution Spectroscopic Observations from 2018 to 2023
di: Qin, Mingfeng, et al.
Pubblicazione: (2025)

Revisiting the Li abundances of Stars with and without Detected Planets from the High Resolution Spectroscopy
di: Qin, Jinxiao, et al.
Pubblicazione: (2025)

Discovery of a new IW And-type dwarf nova with both tilted disk and tidal instability
di: Sun, Yongkang, et al.
Pubblicazione: (2024)

Evaluating the chromospheric structure model of AD Leo using RH1.5D and magnetic field data
di: Liu, Shuai, et al.
Pubblicazione: (2025)

Non-adiabatic Effect on Convective Mode
di: Ando, Hiroyasu
Pubblicazione: (2026)

Global Turbulent Solar Convection: a Numerical Path Investigating Key Force Balances in the context of the Convective Conundrum
di: Noraz, Quentin, et al.
Pubblicazione: (2025)

Formation Channels of Magnetars
di: Hu, Rui-Chong, et al.
Pubblicazione: (2025)

Many Roads Lead to Lithium: Formation Pathways For Lithium-Rich Red Giants
di: Sayeed, Maryum, et al.
Pubblicazione: (2023)

New symbiotic stars or candidates in LAMOST low resolution spectra
di: Zhao, Yabing, et al.
Pubblicazione: (2025)

A Tale of Two Origins: In-Situ versus Accreted Nitrogen-Rich Field Stars in the MW
di: Qiao, Yi, et al.
Pubblicazione: (2026)

The true nature of HE0057-5959, the most metal-poor Li-rich star
di: Mucciarelli, A., et al.
Pubblicazione: (2024)

Formation Channels of Gravitationally Resolvable Double White Dwarf Binaries Inside Globular Clusters
di: Hellström, Lucas, et al.
Pubblicazione: (2025)

Light Curve Models of Convective Common Envelopes
di: Noughani, N., et al.
Pubblicazione: (2024)

The Tip of Red Giant Branch Distances to Nearby Dwarf Galaxies WLM and Sextans A with JWST
di: Yan, Ziming, et al.
Pubblicazione: (2025)

Enhanced extra mixing in low-mass stars approaching the RGB tip and the problem of Li-rich red-clump stars
di: Denissenkov, Pavel A., et al.
Pubblicazione: (2023)

Evidence that Mass Loss on the Red Giant Branch Decreases with Metallicity
di: Li, Yaguang
Pubblicazione: (2025)

Exploring the convective core of the high-amplitude $δ$ Scuti star TIC 120857354 with asteroseismology
di: Chen, Xinghao, et al.
Pubblicazione: (2024)