GC/C/IRMS chromatogram of the 12Â M HCl-hydrolyzed hot-water extracts of the Piv/iPr amino acid esters in Y-980115. The subgraph (a) shows the magnified region with the alanine and glycine peaks. The single-ion traces GC/MS chromatograms of (b) Y-980115 and (c) amino acid standard mixture of the same region as shown in (a) indicate that no coeluting compounds were present that could have interfered the IRMS analysis of Y-980115 and that only alanine and glycine are the main nitrogen-bearing compounds in the region
The Ninth Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites / Hayabusa, Wed. 5...
Stable hydrogen, carbon, and nitrogen isotopic ratios (oD, 013C, and olSN) of organic compounds can ...
The combined volatile bases (ammonia, aliphatic amines, and possibly other bases), ammonia, amino ac...
Indigenous amino acids have been found indigenous all 8 carbonaceous chondrite groups. However, the ...
CR chondrites are among the most primitive meteorites. In this paper, we report the first measuremen...
AbstractWe determined the amino acid abundances and enantiomeric compositions of the Antarctic CI1 c...
Amino acid analyses of the Antarctic CM2 chondrites Allan Hills (ALH) 83100 and Lewis Cliff (LEW) 90...
International audienceLaboratory experiments that simulate the photo- and thermo-chemistry of extrat...
Supplementary data to the paper: 'Bulk mineralogy, water abundance, and hydrogen isotope composition...
We determined the abundances and enantiomeric compositions of amino acids in Sutter’s Mill fragment ...
The Yamato-74662.23 meteorite, a carbonaceous chondrite (C2), was examined for amino acids. The mete...
The carbonaceous chondrites contain significant amounts of carbon- and nitrogen-bearing components, ...
The abundances, distributions, enantiomeric ratios, and carbon isotopic compositions of amino acids ...
The carbonaceous chondrites are intriguing and unique in the sense that they are the only rocks that...
Amino acids, the building blocks of proteins, have been found to be indigenous in most of the carbon...
The Ninth Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites / Hayabusa, Wed. 5...
Stable hydrogen, carbon, and nitrogen isotopic ratios (oD, 013C, and olSN) of organic compounds can ...
The combined volatile bases (ammonia, aliphatic amines, and possibly other bases), ammonia, amino ac...
Indigenous amino acids have been found indigenous all 8 carbonaceous chondrite groups. However, the ...
CR chondrites are among the most primitive meteorites. In this paper, we report the first measuremen...
AbstractWe determined the amino acid abundances and enantiomeric compositions of the Antarctic CI1 c...
Amino acid analyses of the Antarctic CM2 chondrites Allan Hills (ALH) 83100 and Lewis Cliff (LEW) 90...
International audienceLaboratory experiments that simulate the photo- and thermo-chemistry of extrat...
Supplementary data to the paper: 'Bulk mineralogy, water abundance, and hydrogen isotope composition...
We determined the abundances and enantiomeric compositions of amino acids in Sutter’s Mill fragment ...
The Yamato-74662.23 meteorite, a carbonaceous chondrite (C2), was examined for amino acids. The mete...
The carbonaceous chondrites contain significant amounts of carbon- and nitrogen-bearing components, ...
The abundances, distributions, enantiomeric ratios, and carbon isotopic compositions of amino acids ...
The carbonaceous chondrites are intriguing and unique in the sense that they are the only rocks that...
Amino acids, the building blocks of proteins, have been found to be indigenous in most of the carbon...
The Ninth Symposium on Polar Science/Ordinary sessions: [OA] Antarctic meteorites / Hayabusa, Wed. 5...
Stable hydrogen, carbon, and nitrogen isotopic ratios (oD, 013C, and olSN) of organic compounds can ...
The combined volatile bases (ammonia, aliphatic amines, and possibly other bases), ammonia, amino ac...