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  4. The effect of impact obliquity on shock heating in planetesimal collisions
 
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The effect of impact obliquity on shock heating in planetesimal collisions
File(s)
Davison et al-Meteorit Planet Sci_2014.pdf (645.48 KB)
Published version
OA Location
http://onlinelibrary.wiley.com/doi/10.1111/maps.12394/abstract
Author(s)
Davison, TM
Cielsa, FJ
Collins, GS
Elbeshausen, D
Type
Journal Article
Date Issued
2014-11-20
Date Acceptance
2014-10-13
Citation
Meteoritics & Planetary Science, 2014, 49 (12), pp.2252-2265
URI
http://hdl.handle.net/10044/1/31879
DOI
https://www.dx.doi.org/10.1111/maps.12394
ISSN
1086-9379
Publisher
Wiley
Start Page
2252
End Page
2265
Journal / Book Title
Meteoritics & Planetary Science
Volume
49
Issue
12
Copyright Statement
© 2014 The Authors. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
License URL
http://creativecommons.org/licenses/by/4.0/
Sponsor
Science and Technology Facilities Council (STFC)
Identifier
http://hdl.handle.net/10044/1/30734
Grant Number
ST/J001260/1
Subjects
Science & Technology
Physical Sciences
Geochemistry & Geophysics
MELT PRODUCTION
SCALING LAWS
SIMULATIONS
TARGETS
FRAGMENTATION
ASTEROIDS
CRATERS
ORIGIN
0201 Astronomical And Space Sciences
0402 Geochemistry
0403 Geology
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