The planetesimal bow shock model for chondrule formation: A more quantitative assessment of the standard (fixed Jupiter) case
Article first published online: 8 NOV 2012
© The Meteoritical Society, 2012
Meteoritics & Planetary Science
Volume 47, Issue 11, pages 1715–1727, November 2012
How to Cite
HOOD, L. L. and WEIDENSCHILLING, S. J. (2012), The planetesimal bow shock model for chondrule formation: A more quantitative assessment of the standard (fixed Jupiter) case. Meteoritics & Planetary Science, 47: 1715–1727. doi: 10.1111/maps.12006
- Issue published online: 21 DEC 2012
- Article first published online: 8 NOV 2012
- (Received 24 January 2012; revision accepted 16 September 2012)
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