Abstract
Molecular outflows can be modelled as environmental material entrained into high velocity stellar jets. Even though models of this entrainment process are at this time quite uncertain, a few preliminary theoretical efforts have been made. Three different models are discussed, in which the molecular outflows are identified with the turbulent mixing layer at the edge of a jet, with a turbulent envelope (driven by a large number of internal working surfaces in the jet) and with the wake of one working surface.
Similar content being viewed by others
References
Bachiller, R. and Gómez-Gonzáles, J.: 1992,Astron. Astrophys. Rev. 3, 257.
Cabrit, S.: 1994, inStellar Jets and Bipolar Outflows, eds. L. Errico and A. A. Vittone, Kluwer, Dordrecht, in press.
Cantó, J. and Raga, A. C.: 1991,Astrophys. J. 372, 646.
Lada, C.: 1985,Ann. Rev. Astron. Astrophys. 23, 267.
Masson, C. R. and Chernin, L. M.: 1993,Astrophys. J. 414, 230.
Mundt, R., Brugel, E. W. and Bührke, T.: 1987,Astrophys. J. 319, 275.
Pudritz, R.: 1988, inGalactic and Extragalactic Star Formation, eds. R. Pudritz and M. Fich, NATO ASI Series, Kluwer, Dordrecht, p. 135.
Raga, A. C.: 1991,Astron. J. 101, 1472.
Raga, A. C. and Cabrit, S.: 1993,Astron. Astrophys. 278, 267.
Raga, A. C., Cantó, J., Calvet, N., Rodríguez, L. F. and Torrelles, J. M.: 1993,Astron. Astrophys. 276, 539.
Raga, A. C., Cantó, J., Binette, L. and Calvet, N.: 1990,Astrophys. J. 364, 601.
Raga, A. C. and Kofman, L.: 1992,Astrophys. J. 386, 222.
Reipurth, B. and Olberg, M.: 1991,Astron. Astrophys. 246, 535.
Richer, J. S., Hills, R. E. and Padman, R.: 1992,Mon. Not. Roy. Astr. Soc. 254, 535.
Snell, R. L., Bally, J., Strom, S. E. and Strom, K. M.: 1985,Astrophys. J. 290, 587.
Stahler, S. W.: 1994, inAstrophysical Jets, ed. M. Livio, C. O'Dea and D. Burgarella, Cambridge Univ. Press, in press.
Wilson, M.: 1984,Mon. Not. Roy. Astr. Soc. 209, 923.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Raga, A.C. Coupled stellar jet/molecular outflow models. Astrophys Space Sci 216, 105–112 (1994). https://doi.org/10.1007/BF00982476
Issue Date:
DOI: https://doi.org/10.1007/BF00982476