Hydrodynamical models of presolar nebula formation

Details Hydrodynamical models of presolar nebula formation Hydrodynamical models of presolar nebula formation

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982icar...51..623b&link_type=abstract

Icarus, vol. 51, Sept. 1982, p. 623-632.

Astronomy and Astrophysics

Astronomy

16

Astronomical Models, Hydrodynamics, Nebulae, Protostars, Solar System, Binary Stars, Gravitational Collapse, Hierarchies, Stellar Evolution

Scientific paper

Theories of solar system formation often presuppose the existence of the protosun and an accompanying preplanetary nebula. Numerical three-dimensional calculations are presented which demonstrate the possibility of formation of a co-orbital, triple protostellar system, which is unstable to decay to a binary and an ejected single star. The calculations are used to construct a plausible scenario for presolar nebula formation based on a hierarchy of collapse and fragmentation. While this sequence is unlikely to produce many single stars, it remains a possible sequence for the formation of the presolar nebula.

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