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A model of molecular emission in bipolar flows

Published online by Cambridge University Press:  04 August 2017

Sylvie Cabrit  and
Claude Bertout
Sylvie Cabrit
Affiliation:
Institut d'Astrophysique de Paris 98bis Bd Arago 75014 PARIS FRANCE
Claude Bertout
Affiliation:
Institut d'Astrophysique de Paris 98bis Bd Arago 75014 PARIS FRANCE

Abstract

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We present a model of CO J=1→0 line formation in accelerated bipolar outflows. We find that the integrated intensity maps can be divided into four categories, depending on the view angle and the flow opening angle. We then show that no accurate values of the flow parameters can be derived from the CO observations without careful modelling of the outflow properties.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 89 - 92
Copyright
Copyright © Reidel 1987 

References

Bastian, U., Bertout, C., Stenholm, L., Wehrse, R. 1980, Astr. Ap. 86, 105 Google Scholar
Cabrit, S., Bertout, C. 1986, Ap. J. 307, 313 Google Scholar
Goldsmith, P.F., Snell, R.L., Hemeon-Heyer, M., Langer, W.D. 1984, Ap. J. 286, 599 Google Scholar
Lada, C.J. 1985, Ann. Rev. Astr. Ap. 23, 267 Google Scholar
Moriarty-Schieven, G., Snell, R.L., Strom, S.E., Schloerb, F.P., Strom, K.M. 1986, Submitted to Ap. J. Google Scholar