Stellar Clusters and Associations: Convection, Rotation, and Dynamos

By R. Jeffries, E. Totten, J. Stauffer, D. B. Navascues, N. Hambly. 2000

230 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/93ddea1d0732149b5c568a673896b38fd65d6015

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Citations in the corpus

Late-type stars members of young stellar kinematic groups - I. Single stars (2001, methodology): “More complex structures characterized by several longer branches (Sirius, middle, and Pleiades branches) running almost parallel to each other across the UV-plane have been found by Skuljan et al. (1999) in their study of the velocity distribution of stars in the solar neighborhood.”
Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue (2009, background): “A major study of the Hyades cluster as based on the first Hipparcos catalogue was presented by Perryman et al. (1998), and further studies based on the same data by Madsen et al. (2000), Madsen et al. (2001) and de Bruijne et al. (2001).”
The stellar activity-rotation relationship revisited: Dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfs ? (2003, methodology): “…authors have applied such an empirical Rossby number out of its range of applicability (for example, Maggio et al. 1987 have used this function to evaluate τ e for stars of luminosity class IV, or Giampapa et al. 1998 and Randich 2000 for cluster stars younger and redder than the Noyes's dwarfs).”
The Sun in Time: Activity and Environment (2007, background): “All studies find roughly LX/Lbol ∝ P −2 for late-type stars (e.g., Randich 2000).”
THE SEGUE STELLAR PARAMETER PIPELINE. II. VALIDATION WITH GALACTIC GLOBULAR AND OPEN CLUSTERS (2007, methodology): “In total, we obtained SDSS spectroscopy for 1920, 1280, 1280, 1280, and 640 targets, including sky spectra and calibration object spectra, in the fields of M 13, M 15, M 2, NGC 2420, and M 67, respectively.”