The effects of angular momentum play an important role in star formation. However, when a
young star emerges on the Hertzsprung-Russell diagram it is generally rotating slowly. This …

This paper reviews the rich corpus of observational evidence for tidal effects, mostly based
on photometric and radial-velocity measurements. This is done in a period when the study of …

While the strong anticorrelation between chromospheric activity and age has led to the
common use of the Ca ii H and K emission index (R^{\prime} _ {\mathrm {HK}\,}= L …

We propose a simple interpretation of the rotation period data for solar-and late-type stars.
The open cluster and Mount Wilson star observations suggest that rotating stars lie primarily …

ABSTRACT Young (125 Myr), populous (> 1000 members), and relatively nearby, the
Pleiades has provided an anchor for stellar angular momentum models for both younger …

Context. In previous works of this series, we have shown that late B-and early A-type stars
have genuine bimodal distributions of rotational velocities and that late A-type stars lack …

Solar-like stars (M≲ 1.3 M⊙) lose angular momentum through their magnetized winds. The
resulting evolution of the surface rotation period, which can be directly measured …

Aims. The main goal of this work is to measure rotation periods of the M-type dwarf stars
being observed by the CARMENES exoplanet survey to help distinguish radial-velocity …

The angular momentum evolution of low-mass stars. ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS …

Aims. A sample of of B9 to F2-type main sequence single stars has been built from highly
homogeneous parameters determined for a large sample cleansed of objects presenting the …