Fundamental properties of nearby single early B-type stars.¶
Nieva, M., & Przybilla, N. (2014). Fundamental properties of nearby single early B-type stars. 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 sourceQuantitative non-LTE spectroscopy tests the mapping from early-B classifications to masses, radii, luminosities, ages, and evolutionary models.
- … 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:7f021e8428d6 · see in the full table