Starting from the mathematical expression for the Stefan-Boltzmann 6) law: L = 4TR²O$BT*, where ØSe is the Stefan-Boltzmann constant, R is the radius of the star and T is its temperature in Kelvin scale, verify that the isoradius lines in the HR Diagram must be parallel to each other.
Starting from the mathematical expression for the Stefan-Boltzmann 6) law: L = 4TR²O$BT*, where ØSe is the Stefan-Boltzmann constant, R is the radius of the star and T is its temperature in Kelvin scale, verify that the isoradius lines in the HR Diagram must be parallel to each other.
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The isoradius lines are the green lines in the HR diagram
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