⌘+K

Pulse Explore Communities Researchers Journals

Home Communities Explore

January 13, 2012Astronomy and AstrophysicsOpen Access

Impact of rotation and disc lifetime on pre-main sequence lithium depletion of solar-type stars

P. Eggenberger L. Haemmerlé G. Meynet A. Maeder

View Full Paper

Ask AI

Bookmark

Share

Abstract

Aims. We study the influence of rotation and disc lifetime on lithium depletion of pre-main sequence (PMS) solar-type stars.

Discussion

No takes yet. Share an insight, caveat, or question.

Cite This Study

Eggenberger et al. (2012) studied this question.

synapsesocial.com/papers/69dcbeff7873f5f05b133a5d https://doi.org/10.1051/0004-6361/201118432

View Full Paper

Ask AI

Bookmark

Share

Keep reading

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1The Chemical Composition of the SunReview · 2009 · 9,346 citations
2Lithium depletion in solar-like stars: no planet connectionOriginal Research · 2010 · 166 citations
3Lithium depletion and the rotational history of exoplanet host starsOriginal Research · 2008 · 177 citations
4Angular Momentum Transport in Magnetized Stellar Radiative Zones. II. The Solar Spin-downOriginal Research · 1993 · 182 citations
5New pre-main-sequence tracks for M less than or equal to 2.5 solar mass as tests of opacities and convection modelOriginal Research · 1994 · 689 citations

Efficiency of convection and Pre-Main Sequence lithium depletion2003
A MODEL OF MAGNETIC BRAKING OF SOLAR ROTATION THAT SATISFIES OBSERVATIONAL CONSTRAINTS2010
ANGULAR MOMENTUM TRANSPORT IN SOLAR-TYPE STARS: TESTING THE TIMESCALE FOR CORE-ENVELOPE COUPLING2010
A giant magnetic eruption from the asymptotic-giant-branch star Mira AAstronomy and Astrophysics · 2026
Ensemble pulsational characteristics of eclipsing binaries containing β Cep stars observed by the TESS missionAstronomy and Astrophysics · 2026

More from Astronomy and Astrophysics

More from University of Geneva