Figure 6
From: Distributions of CHN compounds in meteorites record organic syntheses in the early solar system
Intensities of the CHN compounds at different micro-spots and overall. (a) CnH2n−6N homologs in the Murchison meteorite. (b) CnH2n−3N2 homologs in the Murchison meteorite. (c) CnH2n−6N homologs in the NWA 801 meteorite. (d) CnH2n−3N2 homologs in the NWA 801 meteorite. Filled colored circles with dotted lines represent the profile from micro-spots. Filled diamonds with solid gray lines represent the profile from the entire region of the samples, shown in percentage intensities.
