C. Pillinger

CM chondrites exhibit the complete petrologic range from type 2 to 1. [Abstract only]

M. Zolensky, D. Mittlefehldt, M. Lipschutz, 1994 .

The origin of chondritic macromolecular organic matter: A carbon and nitrogen isotope study

C. Pillinger, M. Grady, S. Russell, 1998, Meteoritics & planetary science.

The non‐trivial problem of meteorite pairing

D. Sears, C. Pillinger, P. Benoit, 2000 .

The oxygen‐isotopic composition of Earth and Mars

C. Pillinger, I. Franchi, I. Wright, 1999 .

Light dement geochemistry of the Tagish Lake CI2 chondrite: Comparison with CI1 and CM2 meteorites

Ian A. Franchi, Ian Wright, Monica M. Grady, 2002 .

Martian atmospheric carbon dioxide and weathering products in SNC meteorites

M. Grady, R. H. Carr, I. P. Wright, 1985 .

The oxygen isotopic composition of water from Tagish Lake: Its relationship to low‐temperature phases and to other carbonaceous chondrites

C. Pillinger, I. Franchi, I. Wright, 2002 .