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Historical Perspective on Computational Star Formation

Published online by Cambridge University Press:  27 April 2011

Richard B. Larson*
Affiliation:
Department of Astronomy, Yale University, New Haven, CT 06520-8101, USA email: [email protected]
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The idea that stars are formed by gravity goes back more than 300 years to Newton, and the idea that gravitational instability plays a role goes back more than 100 years to Jeans, but the idea that stars are forming at the present time in the interstellar medium is more recent and did not emerge until the energy source of stars had been identified and it was realized that the most luminous stars have short lifetimes and therefore must have formed recently. The first suggestion that stars may be forming now in the interstellar medium was credited by contemporary authors to a paper by Spitzer in 1941 in which he talks about the formation of interstellar condensations by radiation pressure, but then oddly says nothing about star formation. That may be because, as Spitzer later told me, when he first suggested very tentatively in a paper submitted to The Astrophysical Journal that stars might be forming now from interstellar matter, this was considered a radical idea and the referee said it was much too speculative and should be taken out of the paper. So Spitzer removed the speculation about star formation from the published version of his paper.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

References

Basu, S. 1997, ApJ, 485, 240CrossRefGoogle Scholar
Bodenheimer, P. & Sweigart, A. 1968, ApJ, 152, 515CrossRefGoogle Scholar
Bok, B. J. & Reilly, E. F. 1947, ApJ, 105, 255CrossRefGoogle Scholar
Bok, B. J. 1948, in Centennial Symposia, Harvard Observatory Monographs No. 7 (Cambridge, Mass.: Harvard College Observatory), p. 53Google Scholar
Bok, B. J. 1978, PASP, 90, 489CrossRefGoogle Scholar
Christy, R. F. 1966, ApJ, 144, 108CrossRefGoogle Scholar
Hayashi, C. & Nakano, T. 1965, Prog. Theor. Phys., 34, 754CrossRefGoogle Scholar
Hoyle, F. 1953, ApJ, 118, 513CrossRefGoogle Scholar
Jeans, J. H. 1902, Phil. Trans. Roy. Soc., 199, 49Google Scholar
Jeans, J. H. 1929, Astronomy and Cosmogony (Cambridge: Cambridge Univ. Press)Google Scholar
Larson, R. B. 1969a, MNRAS, 145, 271CrossRefGoogle Scholar
Larson, R. B. 1969b, MNRAS, 145, 297CrossRefGoogle Scholar
Larson, R. B. 1972, MNRAS, 156, 437CrossRefGoogle Scholar
Larson, R. B. 1978, MNRAS, 184, 69CrossRefGoogle Scholar
Masunaga, H. & Inutsuka, S. 2000, ApJ, 531, 350CrossRefGoogle Scholar
Nakamura, F., Hanawa, T., & Nakano, T. 1995, ApJ, 444, 770CrossRefGoogle Scholar
Newton, I. 1692, letter to Bentley quoted by Jeans (1929), p. 352Google Scholar
Norman, M. L., Wilson, J. R., & Barton, R. T. 1980, ApJ, 239, 968CrossRefGoogle Scholar
Penston, M. V. 1966, Roy. Obs. Bull., No. 117, 299Google Scholar
Penston, M. V. 1969, MNRAS, 144, 425CrossRefGoogle Scholar
Spitzer, L. Jr. 1941, ApJ, 94, 232CrossRefGoogle Scholar
Spitzer, L. Jr. 1948a, in Centennial Symposia, Harvard Observatory Monographs No. 7 (Cambridge, Mass.: Harvard College Observatory), p. 87Google Scholar
Spitzer, L. Jr. 1948b, Physics Today, Vol. 1, No. 5, p. 7CrossRefGoogle Scholar
Spitzer, L. Jr. 1949, ASP Leaflet, No. 241Google Scholar
Stahler, S. W., Shu, F. H., & Taam, R. E. 1980a, ApJ, 241, 637CrossRefGoogle Scholar
Stahler, S. W., Shu, F. H., & Taam, R. E. 1980b, ApJ, 242, 226CrossRefGoogle Scholar
Whipple, F. L. 1946, ApJ, 104, 1CrossRefGoogle Scholar
Whipple, F. L. 1948, in Centennial Symposia, Harvard Observatory Monographs No. 7 (Cambridge, Mass.: Harvard College Observatory), p. 109Google Scholar
Winkler, K.-H. A. & Newman, M. J. 1980a, ApJ, 236, 201CrossRefGoogle Scholar
Winkler, K.-H. A. & Newman, M. J. 1980b, ApJ, 238, 311CrossRefGoogle Scholar