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Circumstellar radio emission from pre-main sequence stars

Published online by Cambridge University Press:  04 August 2017

Alexander Brown
Alexander Brown*
Affiliation:
Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards, Boulder, Colorado 80309-0440, USA

Abstract

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VLA radio continuum observations have been obtained for a number of pre-main sequence (PMS) stars in Corona Australis, Lupus, Scorpius and Taurus. A variety of PMS sources were detected and for other stars upper limits to the ionized mass loss rates were determined. A strong double source, showing two radio jets, was found associated with an embedded infra-red source in the R CrA molecular cloud. Some of the PMS stars show extended radio emission associated with ionized circumstellar envelopes, even though photoionization by EUV photons is not sufficient to produce the ionized regions.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 63 - 64
Copyright
Copyright © Reidel 1987 

References

Brown, A., Drake, S. A. and Mundt, R. 1986, in Cool Stars, Stellar Systems, and the Sun, eds. Zeilik, M. and Gibson, D. M., Lecture Notes in Physics No. 254 (Springer-Verlag: Berlin), p. 451.CrossRefGoogle Scholar
Brown, R. L. and Zuckerman, B. 1975, Ap. J., 202, L125.CrossRefGoogle Scholar
Kuin, N. P. M. 1986, in Cool Stars, Stellar Systems, and the Sun, eds. Zeilik, M. and Gibson, D. M., Lecture Notes in Physics No. 254 (Springer-Verlag: Berlin), p. 466.Google Scholar
Lago, M. T. V. T. 1984, Mon. Not. R. astr. Soc., 210, 323.Google Scholar
Taylor, K. N. R. and Storey, J. W. V. 1984, Mon. Not. R. astr. Soc., 209, 5p.CrossRefGoogle Scholar