Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...268..381c&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 268, May 1, 1983, p. 381-384. Research supported by the Robert A. Welch Fou
Astronomy and Astrophysics
Astrophysics
22
Abundance, Interstellar Matter, Molecular Clouds, Nuclear Fusion, Radioactive Isotopes, Solar System, Supernovae, Evolution (Development), Hydrogen Clouds, Iodine Isotopes, Isotope Effect, Mass Distribution, Meteoritic Composition, Palladium, Phase Transformations, Plutonium Isotopes, Radioactive Decay
Scientific paper
A new class of models is advanced for interpreting the relationship of radioactive abundances in the early solar system to their average concentration in the interstellar medium. The model assumes that fresh radioactivities are ejected from supernovae into the hot interstellar medium, and that the time scales for changes of phase into molecular clouds determine how much survives for formation therein of our solar system. A more realistic and physically motivated understanding of the low observed concentrations of 129I, 244Pu, and 107Pd may result.
No associations
LandOfFree
Extinct radioactivities - A three-phase mixing model does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Extinct radioactivities - A three-phase mixing model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extinct radioactivities - A three-phase mixing model will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1585481