Add to ORKGStellar Magnetism, eds. C. Neiner, J.-P. Zahn, EAS Publication Series 2008I review the development of ideas regarding the angular momentum evolution of solar-type stars, from the early 60's to the most recent years. Magnetic fields are the central agent that dictates the rotational evolution of solar-type stars, both during the pre-main sequence, through star-disk magnetic coupling, and during the main sequence, through magnetized winds. Key theoretical developments as well as important observational results are summarized in this review
This is the final version. Available from American Astronomical Society via the DOI in this record.T...
We review the theoretical efforts to understand why pre-main-sequence stars spin much more slowly th...
Stellar rotation plays an important role in maintaining the magnetic fields inside the stellar inter...
Stellar Magnetism, eds. C. Neiner, J.-P. Zahn, EAS Publication Series 2008I review the development o...
Today, the generation of magnetic fields in solar‐type stars and its relation to activity and rotati...
Magnetic field is playing an important role at all stages of star evolution from star formation to t...
The surface rotation rates of young solar-type stars vary rapidly with age from the end of the pre-m...
This is the author accepted manuscript. The final version is available from the publisher via the DO...
VS acknowledges support from a Science & Technology Facilities Council (STFC) post-doctoral fellowsh...
AAV acknowledges support from a Royal Astronomical Society Fellowship and from the Swiss National Sc...
Today, one of the greatest challenges concerning the Ap/Bp stars is to understand the origin of thei...
International audienceContext. The early pre-main sequence phase during which solar-mass stars are s...
The solar magnetic field is generated and sustained through an internal dynamo. In stars, this proce...
After their formation, stars slow down their rotation rates by the removal of angular momentum from ...
We investigate how the observed large-scale surface magnetic fields of low-mass stars (̃0.1-2M⊙), re...
This is the final version. Available from American Astronomical Society via the DOI in this record.T...
We review the theoretical efforts to understand why pre-main-sequence stars spin much more slowly th...
Stellar rotation plays an important role in maintaining the magnetic fields inside the stellar inter...
Stellar Magnetism, eds. C. Neiner, J.-P. Zahn, EAS Publication Series 2008I review the development o...
Today, the generation of magnetic fields in solar‐type stars and its relation to activity and rotati...
Magnetic field is playing an important role at all stages of star evolution from star formation to t...
The surface rotation rates of young solar-type stars vary rapidly with age from the end of the pre-m...
This is the author accepted manuscript. The final version is available from the publisher via the DO...
VS acknowledges support from a Science & Technology Facilities Council (STFC) post-doctoral fellowsh...
AAV acknowledges support from a Royal Astronomical Society Fellowship and from the Swiss National Sc...
Today, one of the greatest challenges concerning the Ap/Bp stars is to understand the origin of thei...
International audienceContext. The early pre-main sequence phase during which solar-mass stars are s...
The solar magnetic field is generated and sustained through an internal dynamo. In stars, this proce...
After their formation, stars slow down their rotation rates by the removal of angular momentum from ...
We investigate how the observed large-scale surface magnetic fields of low-mass stars (̃0.1-2M⊙), re...
This is the final version. Available from American Astronomical Society via the DOI in this record.T...
We review the theoretical efforts to understand why pre-main-sequence stars spin much more slowly th...
Stellar rotation plays an important role in maintaining the magnetic fields inside the stellar inter...