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Symposium Summary: Fragmentation and Star Formation in Molecular Clouds

Published online by Cambridge University Press:  03 August 2017

A. E. Glassgold
A. E. Glassgold*
Affiliation:
New York University, New York, NY 10463, U.S.A.

Extract

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This Symposium on fragmentation and star formation has dealt with the heart of the study of molecular clouds, which is how they form stars. This problem is one of the most profound and challenging problems in all of astrophysics. The complexity of the interstellar medium adds to its difficulty and we cannot expect a quick and easy solution. Nonetheless, the reports presented at this Symposium indicate that substantial progress is being made in this field.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 379 - 386
Copyright
Copyright © Kluwer 1991 

References

Adams, F.C., Lada, C.J., and Shu, F.H. 1987, Ap.J. 312, 836.Google Scholar
Black, J.H. 1990, this meeting.Google Scholar
Boulanger, F. 1990, this meeting.Google Scholar
Courtes, G. 1955, in “Gas Dynamics of Cosmic Clouds”, (Interscience, 1955), p.131.Google Scholar
Draine, B.T. 1990, this meeting.Google Scholar
Elmegreen, B.G., 1990, this meeting.Google Scholar
Evans, N.J. II and Lada, E.A., 1990, this meeting.Google Scholar
Falgarone, E., 1990, this meeting.Google Scholar
Falgarone, E. and Phillips, T.G., 1990, this meeting.Google Scholar
Feldt, C. and Wendker, H.J. 1990, this meeting.Google Scholar
Heiles, C. 1990, this meeting.Google Scholar
Joncas, G. 1990, this meeting.Google Scholar
Keene, J. 1990, this meeting.Google Scholar
Keene, and Masson, C.R. 1990, Ap.J. 355, 635.Google Scholar
Keto, E.R., Lattanzio, J.C., and Monaghan, J.J. (1990), this meeting.Google Scholar
Lada, E.A. 1990, thesis, Univ. of Texas. Google Scholar
Lada, C.J. 1985, Ann. Rev. Astr. and Ap., 23, 267.Google Scholar
Lada, C.L. and Shu, F.H. 1990, Science, 248, 564.Google Scholar
Larson, R.B. 1990, this meeting.Google Scholar
Larson, R.B. 1980, M.N.R.A.S. 186, 479.Google Scholar
Myers, P.C., 1988, in “Interstellar Processes”, Eds. Hollenbach, D.J. and Thronson, H.A., (Reidel), p.71.Google Scholar
Myers, P.C., 1990, this meeting.Google Scholar
O'Dell, C.R. and Castaneda, O.O. 1987, Ap.J. 317, 686.Google Scholar
O'Dell, C.R. 1990, this meeting.Google Scholar
Scalo, J.M. 1988, in “Interstellar Processes”, Eds. Hollenbach, D.J. and Thronson, H.A., (Reidel), p.349.Google Scholar
Shu, F.H., Adams, F., and Lizano, S. 1987, Ann. Rev. Astr. and Ap., 255, 23.Google Scholar
Smith, M.D., Brand, P.W.J.L., and Moorhouse, A. 1990, this meeting.Google Scholar
Stutzki, J. 1990, this meeting Google Scholar
Stutzki, J. and Gusten, R. 1990, Ap.J. 356, 513.Google Scholar
Thaddeus, P. 1990, this meeting.Google Scholar
Welch, W.J. et al., 1987, Science 238, 1550.Google Scholar