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The Evolution of Flows and Protostars

Published online by Cambridge University Press:  25 May 2016

Philippe André*
Affiliation:
CEA Service d'Astrophysique, Centre d'Etudes de Saclay, F-91191 Gif-sur-Yvette Cedex, France

Abstract

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In this paper, I summarize the key properties of Class 0 protostars, discuss the observational evidence for a decline of outflow/inflow power with evolutionary stage, point out a possible connection with the initial conditions of fast protostellar collapse, and suggest a new collapse scenario in regions of induced, multiple star formation. The main thesis put forward here is that Class 0 objects have unusually powerful outflows because they accrete at a substantially higher rate than their Class I descendants.

Type
V. Low- and High-Mass Protostars and Their Environment
Copyright
Copyright © Kluwer 1997 

References

Abergel, A., Bernard, J.P., Boulanger, F. et al. 1996, A&A, 315, L329.Google Scholar
Andre, P., Montmerle, T. 1994, ApJ 420, 837 - AM94.Google Scholar
Andre, P., Ward-Thompson, D., Barsony, M., 1993, ApJ, 406, 122 - AWB93.Google Scholar
Andre, P., Ward-Thompson, D., Motte, F. 1996, A&A, 314, 625 - AWM96.Google Scholar
Bachiller, R. 1996, A.R.A.A., 34, 111.Google Scholar
Bontemps, S., Andre, P., & Ward-Thompson, D. 1995, A&A, 297, 98.Google Scholar
Bontemps, S., Andre, P., Terebey, S. & Cabrit, S. 1996, A&A, 311, 858 - BATC.Google Scholar
Boss, A.P. 1995, ApJ 439, 224.CrossRefGoogle Scholar
Ferreira, J., Pelletier, G. 1995, A&A 295, 807.Google Scholar
Foster, P.N., Chevalier, R.A. 1993, ApJ 416, 303 - FC93.Google Scholar
Greene, T.P., Wilking, B.A., André, P., Young, E.T., Lada, C.J. 1994, ApJ 434, 614.Google Scholar
Henning, Th., Michel, B., & Stognienko, R. 1995, Planet. Space Sci., 43, 1333.CrossRefGoogle Scholar
Henriksen, R.N. 1994, in: Montmerle, T., Lada, C.J., Mirabel, I.F., Trân Thanh Van, J. (eds.) The Cold Universe. Editions Frontières, p.241H94.Google Scholar
Henriksen, R.N., Andre, P., & Bontemps, S. 1997, A&A, in press.Google Scholar
Kenyon, S.J., Calvet, N., & Hartmann, L. 1993, ApJ 414, 676.Google Scholar
Lada, C.J. 1987, in: Peimbert, M., Jugaku, J. (eds.) Star Forming Regions. IAU 115, p.1.Google Scholar
Ladd, E.F., Adams, F.C., Casey, S. et al. 1991, ApJ 382, 555.Google Scholar
Li, S., & Shu, F.H. 1996, ApJ, 472, 211.Google Scholar
Loren, R.B., Wootten, A., 1986, ApJ, 306, 142.Google Scholar
Mezger, P.G., Sievers, A.W., Haslam, C.G.T., et al. 1992, A&A, 256, 631.Google Scholar
Motte, F., André, P., Neri, R. 1996, in: Siebenmorgen, R., Kaufl, H.U. (eds.) The Role of Dust in the Formation of Stars. ESO Astrophysics Symposia. Springer, Berlin, p. 47.CrossRefGoogle Scholar
Motte, F., André, P., Neri, R. 1997, A&A, in preparation (see Poster Proceedings).Google Scholar
Mouschovias, T.M. 1991, in The Physics of Star Formation and Early Stellar Evolution, Eds. Lada, & Kylafis, (Kluwer), p. 449.Google Scholar
Pudritz, R.E., Pelletier, G, & Gomez de Castro, A.I. 1991, in The Physics of Star Formation and Early Stellar Evolution, Eds. Lada, & Kylafis, (Kluwer), p. 539.Google Scholar
Saraceno, P., André, P., Ceccarelli, C., Griffin, M., Molinari, S. 1996, A&A, 309, 827.Google Scholar
Shu, F. 1977, ApJ, 214, 488.Google Scholar
Shu, F.H., Adams, F.C., Lizano, S. 1987, ARA&A 25, 23.Google Scholar
Shu, F., Najita, J., Ostriker, E. et al. 1994, ApJ 429, 781.Google Scholar
Stahler, S.W. 1988, ApJ 332, 804.Google Scholar
Tomisaka, K. 1996, PASJ, 48, L97.Google Scholar
Ward-Thompson, D., Scott, P.F., Hills, R.E., & André, P. 1994, MNRAS, 268, 276.Google Scholar
Whitworth, A., & Summers, D. 1985, MNRAS, 214, 1.Google Scholar
Zuckerman, B., & Becklin, E.E. 1993, ApJ, 414, 793.Google Scholar