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Science (New York, N.Y.)|November 23, 1973
Organic Compounds in Meteorites: They may have formed in the solar nebula, by catalytic reactions of carbon monoxide, hydrogen, and ammoniaE Anders, R Hayatsu, M H StudierProceedings of the National Academy of Sciences of the United States of America|December 1, 1976
Covalently linked chlorophyll a dimer: A biomimetic model of special pair chlorophyllM R Wasielewski, M H Studier, J J KatzScience (New York, N.Y.)|September 26, 1980
Carbynes in meteorites: detection, low-temperature origin, and implications for interstellar moleculesR Hayatsu, R G Scott, M H Studier, et al.Journal of Pharmaceutical Sciences|March 1, 1976
Biosynthesis of deuterated riboflavin: structure determination by NMR and mass spectrometryP L Pluta, H L Crespi, M Klein, et al.Science (New York, N.Y.)|March 14, 1980
Phenolic ethers in the organic polymer of the murchison meteoriteR Hayatsu, R E Winans, R G Scott, et al.Pageof 1