Abstract
Designating a star as of A-type is a result of spectral classification. After separating the peculiar stars from those deemed to be normal using the results of a century of stellar astrophysical wisdom, I define the physical properties of the ”normal” stars. The hotter A stars have atmospheres almost in radiative equilibrium. In the A stars convective motions can be found which increase in strength as the temperature decreases.
Cite
CITATION STYLE
APA
Adelman, S. J. (2004). The physical properties of normal A stars. Proceedings of the International Astronomical Union, 2004(IAUS224), 1–11. https://doi.org/10.1017/s1743921304004314
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