stellar structure wikipedia - EAS
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Stellar structure models describe the internal structure of a star in detail and make predictions about the luminosity, the color and the future evolution of the star. Different classes and ages of stars have different internal structures, reflecting their elemental makeup and energy transport mechanisms. See more
Different layers of the stars transport heat up and outwards in different ways, primarily convection and radiative transfer, but thermal conduction is important in white dwarfs.
Convection is the … See moreThe above simplified model is not adequate without modification in situations when the composition changes are sufficiently rapid. … See more
• Kippenhahn, R.; Weigert, A. (1990), Stellar Structure and Evolution, Springer-Verlag
• Hansen, Carl J.; Kawaler, Steven D.; Trimble, Virginia (2004), Stellar Interiors (2nd ed.), Springer, ISBN 0-387-20089-4 See moreThe simplest commonly used model of stellar structure is the spherically symmetric quasi-static model, which assumes that a star is in a steady state and that it is spherically symmetric. It contains four basic first-order differential equations: two represent how See more
• opacity code retrieved November 2009
• The Yellow CESAM code, stellar evolution and structure Fortran source code
• EZ to Evolve ZAMS Stars a FORTRAN 90 software derived from Eggleton's Stellar Evolution Code, a web-based interface can be found here See moreWikipedia text under CC-BY-SA license Stellar structure by Wikipedia
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