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Herbig-Haro emission in two bipolar reflection nebulae

Published online by Cambridge University Press:  04 August 2017

H. J. Staude ,
Th. Neckel ,
M. Sarcander  and
K. Birkle
H. J. Staude
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-6900 Heidelberg, F.R.G.
Th. Neckel
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-6900 Heidelberg, F.R.G.
M. Sarcander
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-6900 Heidelberg, F.R.G.
K. Birkle
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-6900 Heidelberg, F.R.G.

Abstract

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CCD images show that the reflection nebula associated with PV Cep is bipolar. From spectroscopy of this object as well as of the bipolar Boomerang Nebula we find low excited Herbig-Haro emission and indications for collimated high velocity flows along the polar axes of both nebulae. The central star of the Boomerang Nebula is probably double.

Type
Herbig-Haro Objects
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 181 - 182
Copyright
Copyright © Reidel 1987 

References

Appenzeller, I., Jankovics, I., Östreicher, R.: 1984, Astron. Astrophys. 141, 108 Google Scholar
Cohen, M., Kuhi, L.V., Harlan, E.A., Spinrad, H.: 1981, Astrophys. J. 245, 920 Google Scholar
Levreault, R.M.: 1984, Astrophys. J. 277, 634 Google Scholar
Sarcander, M., Neckel, Th., Elsässer, H.: 1985, Astron. Astrophys. 288, L51 Google Scholar
Wegner, G., Glass, I.S.: 1979, MNRAS 188, 327 Google Scholar