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Nanoscale Variation in Carbonaceous Matter from Primitive Meteorites Revealed by Aberration-Corrected STEM

Published online by Cambridge University Press:  23 September 2015

Bradley T De Gregorio
Affiliation:
Nova Research, Inc., Alexandria, VA USA.
Rhonda M Stroud
Affiliation:
Materials Science and Technology Division, Naval Research Laboratory, Washington, DC USA.
Kate D Burgess
Affiliation:
Materials Science and Technology Division, Naval Research Laboratory, Washington, DC USA. ASEE NRL Postdoctoral Fellowship Program
Conel M. O'D Alexander
Affiliation:
Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC USA.
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Copyright © Microscopy Society of America 2015 

References

[1] Alexander, CMO'D, et al, Geochimica et Cosmochimica Acta 71 (2007). p. 4380.CrossRefGoogle Scholar
[2] Bussman, H, et al,, Science 312 (2006).) (p. 727.CrossRefGoogle Scholar
[3] De Gregorio, BT, et al, Meteoritics & Planetary Science 48 (2013). p. 904.CrossRefGoogle Scholar
[4] De Gregorio, BT, et al, Microscopy and Microanalysis 20(S3) (2014). p. 1694.CrossRefGoogle Scholar
[5] Vollmer, C, et al, Proceedings of the National Academy of Sciences 43 (2014). p. 15338.Google Scholar
[6] Huss, GR, Rubin, AE & Grossman, JN in "Meteorites in the Early Solar System II. , (ed.)", DS Lauretta & HY McSween Jr., (University of Arizona Press, Tucson, AZ) p. 567.Google Scholar
[7] The authors acknowledge funding from NASA Origins Program, Grant NNH14AX71I. Dr. LR Nittler has also contributed essential discussions to this work..Google Scholar
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