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Determination of the effective temperatures OF B, A, and F stars of luminosity classes III–V from the slope of the spectrum in the Balmer continuum

N. A. Sokolov

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Key concepts: Balmer series, Physics, Astrophysics, Stars, Luminosity, Effective temperature, Spectrum (functional analysis), Stellar atmosphere

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Determination of the effective temperatures OF B, A, and F stars of luminosity classes III–V from the slope of the spectrum in the Balmer continuum — Research Paper | ScholarLens