Volume 2 contains the basic physical ideas and laws used in the study of the outer layers of a star including stellar magnitudes, spectra and temperatures, radiative transfer in a stellar atmosphere, line formation, the spectrum of hydrogen, spectral analysis, and available structural components.
Stellar astrophysics. Stellar atmosphere
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π SIMILAR VOLUMES
Volume 2 contains the basic physical ideas and laws used in the study of the outer layers of a star including stellar magnitudes, spectra and temperatures, radiative transfer in a stellar atmosphere, line formation, the spectrum of hydrogen, spectral analysis, and available structural components.
<p>Sects. 12, 13. 89 sequence and that subgiant and fainter stars in globular clusters have ultraviolet excesses. When dealing with stars whose physical properties are imperfectly underΒ stood, such as in globular cluster stars, we cannot rely too heavily on the empiriΒ cal calibration by the kinds