Rotating massive MS stars evolutionary models (Brott+, 2011)

Details Rotating massive MS stars evolutionary models (Brott+, 2011) Rotating massive MS stars evolutionary models (Brott+, 2011)

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35309115b&link_type=abstract

VizieR On-line Data Catalog: J/A+A/530/A115. Originally published in: 2011A&A...530A.115B

Computer Science

Models: Evolutionary, Isochrones, Stars: Dwarfs, Rotational Velocities, Abundances

Scientific paper

Isochrones up to hydrogen exhaustion for various rotational velocities generated from the evolutionary models presented in this paper. Mass Range: 5-60M&sun;, δM: 0.05M&sun; Rotational velocity range: 0-540km/s , δv: 10km/s Ages covered: 0-35Myrs , δt: 0.2Myrs Ages and initial compositions are coded in the file names: Filename Format: aiso_..dat
Evolutionary Models for various initial masses (5-60M&sun;) and initial rotational velocities (0-~550)km/s calculated until after core hydrogen exhaustion. Many models continue until helium ignition. Initial masses and rotational velocities at the zero age main sequence velocities can be read from the filenames Filename Format: f-..track.dat
Chemical mixtures are indicated as "lmc", "smc" or "mw" for Large Magellanic Cloud, Small Magellanic Cloud and Galactic initial compositions, respectively. See the Paper for details.
(4 data files).

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