SPH Calculations of Collisions between Main-Sequence Stars

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dc.creatorRasio, Frederic A.
dc.date1995-12-12
dc.date.accessioned2026-07-07T02:20:36Z
dc.date.available2026-07-07T02:20:36Z
dc.descriptionThe hydrodynamics of collisions and mergers of main-sequence stars is discussed in the light of recent 3-D calculations using the smoothed particle hydrodynamics (SPH) method. Theoretical models for the formation of blue stragglers are reviewed in the context of recent comparisons between the observed properties of blue stragglers in dense globular clusters and the predictions of those models.
dc.descriptionuuencoded compressed postscript, 10 pages including one figure. To appear in IAU Symposium 174, Dynamical Evolution of Star Clusters, eds. P. Hut and J. Makino. Also available from http://ensor.mit.edu/~rasio/
dc.identifierhttps://arxiv.org/abs/astro-ph/9512075
dc.identifierhttp://arxiv.org/abs/astro-ph/9512075
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10259
dc.subjectAstrophysics
dc.titleSPH Calculations of Collisions between Main-Sequence Stars
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