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Astron. Astrophys. 364, 935 (2000)

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Origin of H I clouds in the Local Bubble

I. A hydromagnetic Rayleigh-Taylor instability caused by the interaction between the Loop I and the Local Bubble *

D. Breitschwerdt, M.J. Freyberg and R. Egger

Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, 85740 Garching, Germany (breitsch,mjf,roe@mpe.mpg.de)

Astron. Astrophys. 361, 303-320 (2000)

* Paper dedicated to the memory of Franz D. Kahn

Present address: Department of Astrophysical Sciences, 108 Peyton Hall, Princeton University, Princeton, NJ 08544, USA (breitsch@astro.princeton.edu)

Send offprint requests to: D. Breitschwerdt

Due to an unfortunate error Fig. 5 and Fig. 6 have not been printed in colour. Following this page we reprint the article including coloured Figs. 5 and 6 with its original page numbers to avoid confusion in citation of the article.

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© European Southern Observatory (ESO) 2000

Online publication: January 29, 2001