Overview and current relevance of "Run-away stars as the result of the gravitational collapse of proto-stellar clusters" by Poveda, Ruiz, & Allen (1967)

Details Overview and current relevance of "Run-away stars as the result of the gravitational collapse of proto-stellar clusters" by Poveda, Ruiz, & Allen (1967) Overview and current relevance of "Run-away stars as the result of the gravitational collapse of proto-stellar clusters" by Poveda, Ruiz, & Allen (1967)

Apr 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..39...21a&link_type=abstract

Highlights of the Boletín de los Observatorios de Tonantzintla y Tacubaya (Eds. S. Torres-Peimbert & O. López-Cruz) Revista Mexi

Astronomy and Astrophysics

Astronomy

Stars: Early-Type, Stars: Kinematics And Dynamics, Stars: Protostars

Scientific paper

The mechanism for producing massive runaway stars proposed by A. Poveda,
J. Ruiz and C. Allen, 1967, BOTT, 4, 28, 86, is briefly described. Its
impact over the years and its gradual acceptance as a viable way to
account for such stars are traced. Its current relevance for the
understanding of runaway stars is assessed.

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