Hostname: page-component-586b7cd67f-vdxz6 Total loading time: 0 Render date: 2024-11-24T21:03:14.390Z Has data issue: false hasContentIssue false

Bipolar Flows During Early and Late Phases of Star Evolution

Published online by Cambridge University Press:  19 July 2016

Klaus Volkamer
Affiliation:
German MERU Society, Am Berg 2, D-4516 Bissendorf 2, Germany
Christoph Streicher
Affiliation:
German MERU Society, Am Berg 2, D-4516 Bissendorf 2, Germany

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A mechanism for bipolar flows during early and late phases of star evolution is given, based on recently detected cold dark matter.

Type
4. Late-Type and Other Stars
Copyright
Copyright © Kluwer 1993 

References

Lada, C. J. and Shu, F. F.:1990, ‘The Formation of Sunlike Stars’, SCIENCE 248, 564 Google Scholar
Landolt, H.:1908, ‘Untersuchungen über die fraglichen Änderungen des Gesamtgewichtes chemisch sich umsetzender Körper’, Zeitschr. phys. Chem. 64, 581 Google Scholar
Staude, H. J.:1979, ‘Bipolare Nebel’, Sterne und Weltraum 18, 125 Google Scholar
Volkamer, K.:1981, ‘Existiert eine kosmische Quantelung?’, Sterne und Weltraum 20, 273 Google Scholar
Volkamer, K., Streicher, C., Fagan, J., Walton, K. G., Schenkluhn, H., Marlot, H.: Feb. 1992, ‘Evidence of non-baryonic, cold dark matter from laboratory experiments as disclosed from apparent violations of the law of conservation of mass’, Preprint Google Scholar