The Physical and Theoretical Chemistry of Oxygen

  • David Samuel
  • J. Stauff
  • James A. Fee
  • Bo G. Malmström
  • Tore Vänngård
Part of the Colloquium der Gesellschaft für Biologische Chemie 24.–27. April 1968 in Mosbach/Baden book series (MOSBACH, volume 19)

Abstract

Oxygen, which is the subject of this symposium is probably created during the helium-burning phase of stars. The nuclear reactions involved in the production of the three stable isotopes of oxygen are shown in Fig. 1. The stepwise reactions in which O16, O17 and finally O18 are produced probably occur at temperatures of the order of 108 degrees Kelvin and at very great pressures (i.e. densities of 105 gm per cm) [1].

Fig. 1

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Copyright information

© Springer-Verlag Berlin · Heidelberg 1968

Authors and Affiliations

  • David Samuel
    • 1
  • J. Stauff
    • 2
  • James A. Fee
    • 3
  • Bo G. Malmström
    • 3
  • Tore Vänngård
    • 3
  1. 1.Weizmann Institute of ScienceRehovotIsrael
  2. 2.Institut für physikalische Biochemie und KolloidchemieUniversität FrankfurtDeutschland
  3. 3.Department of BiochemistryUniversity of Göteborg and Chalmers Institute of TechnologyGöteborgSweden

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