Populations of rotating stars I. Models from 1.7 to 15 solar masses at three metallicities and rotation rates from zero to critical.¶
Georgy, C., Ekström, S., Granada, A., Meynet, G., Mowlavi, N., Eggenberger, P., & Maeder, A. (2013). Populations of rotating stars I. Models from 1.7 to 15 solar masses at three metallicities and rotation rates from zero to critical. Astronomy & Astrophysics.
Cited by¶
1 citation across 1 artifact.
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Domain-specific¶
- B-type Main-Sequence Star
- … shape, surface temperature distribution, projected line widths, luminosity, and inferred age; metallicity changes the metal-line criteria; chemical peculiarities change diagnostic line strengths; unresolved companions combine spectra and flux; and evolution across the main-sequence band changes gravity and luminosity.
This sourceEstablishes rotation- and metallicity-dependent evolutionary variation across the early-A and B-star mass regime.
- … shape, surface temperature distribution, projected line widths, luminosity, and inferred age; metallicity changes the metal-line criteria; chemical peculiarities change diagnostic line strengths; unresolved companions combine spectra and flux; and evolution across the main-sequence band changes gravity and luminosity.
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Registry ID ref:46df2abf9ba4 · see in the full table