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The extended infrared radiation from the L1551 bipolar flow, L > 19 L⊙

Published online by Cambridge University Press:  04 August 2017

F.O. Clark ,
R.J. Laureijs ,
G. Chlewicki  and
C.Y. Zhang
F.O. Clark
Affiliation:
Lab. for Space Research P.O.B. 800 9700 AV Groningen The Netherlands Dept. of Phys. and Astronomy University of Kentucky Lexington, KY 40506 U.S.A.
R.J. Laureijs
Affiliation:
Lab. for Space Research P.O.B. 800 9700 AV Groningen The Netherlands
G. Chlewicki
Affiliation:
Lab. for Space Research P.O.B. 800 9700 AV Groningen The Netherlands
C.Y. Zhang
Affiliation:
Lab. for Space Research P.O.B. 800 9700 AV Groningen The Netherlands

Abstract

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The infrared bolometric luminosity of the extended infrared emission from the L1551 flow is estimated as 19 (−4 +10) L⊙. Ultraviolet radiation from the shock associated with the flow appears to heat the surrounding dust. The extended infrared emission raises the total energy requirement for the flow over a 10^4 year lifetime to 10^46–47 ergs. If gravitational in origin, this energy likely originates from a region <10^13 cm. Infrared radiation offers a new probe for interstellar shocks by sampling the ultraviolet halo surrounding the shock.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 69 - 70
Copyright
Copyright © Reidel 1987 

References

Clark, F.O. and Laureijs, R.J., 1986 A.&A. 154, L26.Google Scholar
Draine, B.T. 1983 Ap. J. 270, 519.Google Scholar
Emerson, J.P., Harris, S., Jennings, R.E., Beichman, C.A., Baud, B., Beintema, D.A., Marsden, P.L., and Wesselius, P.R. 1984 Ap. J. Letters 278, L49.CrossRefGoogle Scholar
Hollenbach, D. and McKee, C.F. 1979 Ap. J. Suppl. 41, 555.Google Scholar
Snell, R. 1981 Ap. J. Suppl. 45, 121.Google Scholar
Snell, R. and Schloerb, F.P. 1985 Ap. J. 295, 490.Google Scholar