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High-Velocity Clouds and Galactic Evolution

Published online by Cambridge University Press:  25 May 2016

H. van Woerden ,
U.J. Schwarz ,
R.F. Peletier  and
B.P. Wakker
H. van Woerden
Affiliation:
Kapteyn Institute, University of Groningen, Postbus 800, 9700 AV Groningen, The Netherlands
U.J. Schwarz
Affiliation:
Kapteyn Institute, University of Groningen, Postbus 800, 9700 AV Groningen, The Netherlands
R.F. Peletier
Affiliation:
Kapteyn Institute, University of Groningen, Postbus 800, 9700 AV Groningen, The Netherlands
B.P. Wakker
Affiliation:
Dept. of Astronomy, Univ. of Wisconsin, Madison WI, USA

Extract

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High-velocity clouds (HVCs) are HI clouds deviating strongly from the general Galactic rotation. Their distances, and hence origins, have long remained unknown. However, three major complexes are now known to lie at z > 1 kpc, while two smaller clouds are closer to the plane (Wakker et al. 1995). These incomplete results still allow a variety of origins.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 464
Copyright
Copyright © Kluwer 1996 

References

Schwarz, U.J., Wakker, B.P. van Woerden, H. 1995, A&A 302, 364 Google Scholar
Wakker, B.P., van Woerden, H., Schwarz, U.J., Peletier, R.F., Douglas, N.G., Danly, L., de Boer, K.S. 1995, IAU Symp. 169, in press.CrossRefGoogle Scholar
Wakker, B.P., van Woerden, H., Schwarz, U.J., Peletier, R.F., Douglas, N.G. 1996, A&A (Letters), submitted.Google Scholar