Статья

The Monitor Project: stellar rotation at 13 Myr

E. MorauxUJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, FranceS. A. ArtemenkoCrimean Astrophysical Observatory, p/o Nauchny, 98409 Crimea, UkraineJ. BouvierUJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) UMR 5274, 38041 Grenoble, FranceJ. IrwinHarvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge MA 02138, USAM. IbrahimovUlugh Bek Astronomical Institute of the Uzbek Academy of Sciences, Astronomicheskaya 33, 700052 Tashkent, UzbekistanT. Yu. MagakianByurakan Astrophysical Observatory, 0213 Aragatsotn reg., ArmeniaK. N. GrankinCrimean Astrophysical Observatory, p/o Nauchny, 98409 Crimea, UkraineE. H. NikogossianByurakan Astrophysical Observatory, 0213 Aragatsotn reg., ArmeniaC. CardosoNational Institute for AstrophysicsS. T. HodgkinInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UKS. AigrainAstrophysics, Denys Wilkinson Building, University of Oxford, Oxford OX1 3RH, UKT. A. MovsessianByurakan Astrophysical Observatory, 0213 Aragatsotn reg., Armenia

Astronomy and Astrophysicsjournal2013en

ABI

Аннотация

Aims. We aim at constraining the angular momentum evolution of low-mass stars by measuring their rotation rates when they begin to evolve freely towards the zero-age main sequence (ZAMS), i.e., after the disk accretion phase has stopped.

Темы

Astrophysics and Star Formation Studies Stellar, planetary, and galactic studies Astro and Planetary Science

Идентификаторы

DOI: 10.1051/0004-6361/201321508

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