Inhomogeneous Stellar Models. V. a. Solar Model with Convective Envelope and Inhomogeneous Interior.

view Abstract Citations (60) References (7) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Inhomogeneous Stellar Models. V. a. Solar Model with Convective Envelope and Inhomogeneous Interior. Schwarzschild, M. ; Howard, R. ; Härm, R. Abstract A model for the sun has computed in which account has been taken both of the deep hydrogen convection zone and of the internal inhomogeneity in composition caused by the transmutation of hydrogen during the last five billion years. The model is found to permit good agreement with the analysis of the solar photosphere as regards chemical composition and as regards the depth of the hydrogen convection zone. Furthermore, the model indicates that the sun must have become brighter by nearly 2 mag. during the five billion years. Publication: The Astrophysical Journal Pub Date: January 1957 DOI: 10.1086/146297 Bibcode: 1957ApJ...125..233S full text sources ADS | Related Materials (5) Part 1: 1952ApJ...116..317O Part 2: 1952ApJ...116..463S Part 3: 1953ApJ...118..326S Part 4: 1955ApJ...121..445H Part 6: 1957ApJ...126..208W