Comparison of a theory of sequential fragmentation with the initial mass function of stars

Details Comparison of a theory of sequential fragmentation with the initial mass function of stars Comparison of a theory of sequential fragmentation with the initial mass function of stars

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.122..287b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 122, no. 2, May 1986, p. 287-298.

Astronomy and Astrophysics

Astrophysics

5

Astronomical Models, Fragmentation, Galactic Evolution, Stellar Evolution, Stellar Mass, Boundary Value Problems, Solar System, Stellar Envelopes, Stellar Mass Ejection, Supernovae

Scientific paper

The author has formulated a theory of sequential fragmentation based on his theory of solar system formation. The theory is validated using the data from an explosive aerosolization experiment. Comparison of the fragmentation theory with the initial mass function of stars shows excellent agreement. This agreement does not validate the author's solar system formation theory, but it does add support to it and perhaps more importantly, does not falsify it.

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