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Filtered CCD images of southern Herbig-Haro objects

Published online by Cambridge University Press:  04 August 2017

B. Whitmore ,
D.H.M. Cameron  and
R.F. Warren-Smith
B. Whitmore
Affiliation:
Dept. of Physics & Astronomy University College London Gower Street, London WC1E 6BT
D.H.M. Cameron
Affiliation:
Dept. of Physics & Astronomy University College London Gower Street, London WC1E 6BT
R.F. Warren-Smith
Affiliation:
Physics Department, University of Durham, South Road, Durham DH1 3LE

Extract

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It is currently believed that Herbig-Haro (HH) objects are a consequence of a high-velocity (up to at least 200 km s−1) outflow of material from a young embedded star. These flows can often be detected by deep observations of optical emission lines using CCD cameras.

Type
Herbig-Haro Objects
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 189 - 190
Copyright
Copyright © Reidel 1987 

References

Doptia, M.A., Schwartz, R.D. & Evans, I, 1982, Ap. J. Letts., 263, L77.Google Scholar
Graham, J.A. & Frogel, J.A., 1985, Ap. J., 289, 331.Google Scholar