= Self-Similar Collapse of Isothermal Spheres and Star Formation by Frank H. Shu
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{tag=Work by Frank H. Shu}
https://articles.adsabs.harvard.edu/pdf/1977ApJ...214..488S[Original1977 paper]
By <Frank H. Shu>. The Astrophysical Journal214,488–497. The classical expansion-wave collapse model has an initially isothermal outer envelope and a freely falling inner asymptote. The source paper is cited for the model; no numerical similarity eigenvalue is required for the examination scaling argument.
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