On the origin of close binary and planetary systems

Details On the origin of close binary and planetary systems On the origin of close binary and planetary systems

Publishing date

Oct 1978

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...225..198f&link_type=abstract

Journals

Astrophysical Journal, Part 1, vol. 225, Oct. 1, 1978, p. 198-200.

Science

Astronomy and Astrophysics

Field

Astrophysics

Additional info 2

1

Additional info 3

Binary Stars, Planetary Evolution, Planetary Systems, Solar System, Angular Momentum, Early Stars, Stellar Rotation, Stellar Spectra

Type

Scientific paper

Abstract

The angular momenta of close binary and planetary systems suggests that
such systems may form by a similar process, and that this process may
involve the rotational instability of a primary condensation. The
frequency of occurrence of planetary systems may therefore be
essentially independent of the spectral type of the central star.

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