phenomenon 52.17 The Hertzsprung–Russell diagram

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phenomenon 52.17: The Hertzsprung–Russell diagram52.17equation 68.2: eq:bb-stefan-boltzmann68.2equation 52.23: eq:stellar-homology-luminosity52.23phenomenon 52.12: The mass–luminosity relation52.12proof : ch:11-stellar-structure-nucleosynthesis@proof-13proofproposition 52.9: Radiative diffusion52.9equation 52.2: eq:stellar-hydrostatic52.2equation 52.17: eq:stellar-radiative-gradient52.17proposition 52.1: Hydrostatic equilibrium of a self-gravitating sphere52.1proof : ch:11-stellar-structure-nucleosynthesis@proof-8proof

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cites Über die Verwendung photographischer effektiver Wellenlängen zur Bestimmung von Farbenäquivalenten derived parts/05-general-relativity-cosmology/11-stellar-structure-nucleosynthesis.tex:1172
cites Relations Between the Spectra and other Characteristics of the Stars ast; derived parts/05-general-relativity-cosmology/11-stellar-structure-nucleosynthesis.tex:1172
depends_on eq:bb-stefan-boltzmann declared parts/05-general-relativity-cosmology/11-stellar-structure-nucleosynthesis.tex:1176
depends_on eq:stellar-homology-luminosity declared parts/05-general-relativity-cosmology/11-stellar-structure-nucleosynthesis.tex:1176
depends_on The mass–luminosity relation declared parts/05-general-relativity-cosmology/11-stellar-structure-nucleosynthesis.tex:1176
proves ch:11-stellar-structure-nucleosynthesis@proof-13 declared parts/05-general-relativity-cosmology/11-stellar-structure-nucleosynthesis.tex:1180