ChandraWD

planning

Code to produce models of white dwarf stars

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Description

ChandraWD solves the hydrostatic equilibrium equation using degenerate gas equations of state. It produces models of the internal structure of white dwarf stars.

ChandraWD Web Site

Categories

Astronomy

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Additional Project Details

Intended Audience

Science/Research

User Interface

Console/Terminal

Programming Language

C++

Registered

2012-04-15
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