Stellar Rotation in Young Clusters: The First 4 Million Years
By L. Rebull, S. Wolff, S. Strom. 2004
149 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/7eb9574a20fda3b4f8706d4e6a7cd795b5cd0337
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In Astronomy and Astrophysics
Citations in the corpus
- Hipparcos distance estimates of the Ophiuchus and the Lupus cloud complexes (2008, methodology): “Quoted values for the ρ-Ophiuchi cloud are in the range 120–165 pc, as recently summarized by Rebull et al. (2004).”
- Accretion-powered Stellar Winds. II. Numerical Solutions for Stellar Wind Torques (2008, background): “Large data sets for the spins of TTSs in star formation regions and clusters of different ages (see Rebull et al. 2004, for a compilation) show that approximately half of the stars are rotating rapidly and do seem to spin up as expected as they approach zero-age main sequence (Vogel & Kuhi 1981;…”
- FIRST RESULTS FROM HIGH ANGULAR RESOLUTION ALMA OBSERVATIO NS TOWARD THE HL TAU REGION (2015, methodology): “In this paper we adopt the standard mean distance to Taurus of 140 pc (Rebull et al. 2004) for the HL Tau region20.”
- Improved angular momentum evolution model for solar-like stars (2013, background): “While the evidence for PMS rotational regulation is not recent (see, Edwards et al. 1993; Bouvier et al. 1993; Rebull et al. 2004), many theoretical advances have been made in the last years highlighting the impact of the accretion/ejection phenomenon on the angular momentum evolution of young suns…”
- STRUCTURE AND EVOLUTION OF PRE-MAIN-SEQUENCE CIRCUMSTELLAR DISKS (2009, methodology): “Ongoing CARMA development and operations are supported by the National Science Foundation under a cooperative agreement, and by the CARMA partner universities 2 130±15 pc respectively (see Rebull et al. 2004).”