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Modeling the strings in the outer regions of η Carinae

Published online by Cambridge University Press:  26 May 2016

Matt P. Redman ,
John Meaburn  and
Anthony J. Holloway
Matt P. Redman
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
John Meaburn
Affiliation:
Jodrell Bank Observatory, University of Manchester, Macclesfiled SK11 9DL, UK
Anthony J. Holloway
Affiliation:
Jodrell Bank Observatory, University of Manchester, Macclesfiled SK11 9DL, UK

Abstract

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The narrow high-speed optical filaments emerging from the Homunculus of η Carinae are modelled as resulting from the passage of ballistic ‘bullets’ of material through the dense circumstellar environment. In this explanation, the string is the decelerating flow of ablated gas from the bullet. Many of the observed properties of the strings are accounted for in this simple model.

Type
Part 4. Feedback from Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 736 - 737
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Currie, D., Le Mignant, D., Svensson, B., et al. 2000, ESO Messenger 102, 25.Google Scholar
Meaburn, J., Wolstencroft, R.D., Walsh, J.R. 1987, A&A 181, 333.Google Scholar
Redman, M. P., Meaburn, J., Holloway, A.J. 2002, MNRAS 332, 754.Google Scholar
Soker, N. 2001, ApJ 377, 672.Google Scholar
Weis, K., Duschl, W.J., Chu, Y.-H. 1999, A&A 349, 467.Google Scholar