Observational studies of stellar rotation
arXiv:1307.2891 · doi:10.1051/eas/1362005
Abstract
This course reviews the rotational properties of non-degenerate stars as observed from the protostellar stage to the end of the main sequence. It includes an introduction to the various observational techniques used to measure stellar rotation. Angular momentum evolution models developed over the mass range from the substellar domain to high-mass stars are briefly discussed
26 pages, 4 figures. To appear in the Proceedings of the Evry Schatzman School 2012 of PNPS and CNRS/INSU on the "Role and mechanisms of angular momentum transport during the formation and early evolution of stars", Eds. P.Hennebelle and C.Charbonnel
References in corpus (16)
- Large-scale magnetic topologies of late M dwarfs
- Imaging the Surface of Altair
- Interferometric Observations of Rapidly Rotating Stars
- Chromospheric Activity, Rotation, and Rotational Braking in M and L Dwarfs
- Accretion funnels onto weakly magnetized young stars
- Lithium depletion and the rotational history of exoplanet host stars
- Rotation and accretion of very low mass objects in the SigmaOri cluster
- A Correlation Between Pre-Main Sequence Stellar Rotation Rates and IRAC Excesses in Orion
- Rotational Velocities For B0-B3 Stars in 7 Young Clusters: Further Study of the Relationship between Rotation Speed and Density in Star-Forming Regions
- Powerful Winds from Low-Mass Stars: V374 Peg
- Accretion-Powered Stellar Winds III: Spin Equilibrium Solutions
- The Monitor project: Rotation periods of low-mass stars in M50
- Magnetocentrifugally Driven Flows from Young Stars and Disks. VI. Accretion with a Multipole Stellar Field
- The Monitor project: Rotation of low-mass stars in the open cluster NGC 2547
- Projected Rotational Velocities and Stellar Characterization of 350 B Stars in the Nearby Galactic Disk
- Impact of internal gravity waves on the rotation profile inside pre-main sequence low-mass stars
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- CoRoT 223992193: Investigating the variability in a low-mass, pre-main sequence eclipsing binary with evidence of a circumbinary disk
- Even More Rapidly Rotating Pre-Main Sequence M Dwarfs with Highly Structured Light Curves: An Initial Survey in the Lower Centaurus-Crux and Upper Centaurus-Lupus Associations
- Projected Rotational Velocities and Fundamental Properties of Low-Mass Pre-Main Sequence Stars in the Taurus-Auriga Star Forming Region
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- Characterization of Exoplanet-Host Stars
- Empirical Constraints on Core Collapse Supernova Yields using Very Metal Poor Damped Lyman Alpha Absorbers
- Understanding the angular momentum evolution of T Tauri and Herbig Ae/Be stars
- The Primordial Solar wind as a Sculptor of Terrestrial Planet Formation
- WASP 0639-32: a new F-type subgiant/K-type main-sequence detached eclipsing binary from the WASP project
- Stellar rotation effects in polarimetric microlensing
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- A Data-Driven Technique for Measuring Stellar Rotation
- Rotation of planet-harbouring stars
- Dynamic Photometric Variability in Three Young Brown Dwarfs in Taurus: Detection of Optical Flares with TESS data