Theoretical mass loss rates of cool main-sequence stars
Open Access
- 2 November 2006
- journal article
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 463 (1) , 11-21
- https://doi.org/10.1051/0004-6361:20066486
Abstract
Astronomy & Astrophysics (A&A) is an international journal which publishes papers on all aspects of astronomy and astrophysicsKeywords
All Related Versions
This publication has 51 references indexed in Scilit:
- The influence of stellar wind conditions on the detectability of planetary radio emissionsAstronomy & Astrophysics, 2005
- A Hot Wind from the Classical T Tauri Stars: TW Hydrae and T TauriThe Astrophysical Journal, 2005
- The effect of tidal locking on the magnetospheric and atmospheric evolution of “Hot Jupiters”Astronomy & Astrophysics, 2004
- Stellar Coronal AstronomySpace Science Reviews, 2003
- The Faint Young Sun Paradox: An observational test of an alternative solar modelGeophysical Research Letters, 2000
- Constraints on the FIP Mechanisms from Solar Wind Abundance DataSpace Science Reviews, 1998
- Standard Solar CompositionSpace Science Reviews, 1998
- A Relationship between Mean Rotation Period in Lower Main-Sequence Stars and Its Observed RangeThe Astrophysical Journal, 1996
- The solar wind shock terminationAdvances In Space Research, 1986
- Magnetic acceleration of winds from solar-type starsThe Astrophysical Journal, 1976