Disk heating and stellar migration in galaxies

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dc.creatorBinney, J. J.
dc.creatorSellwood, J. A.
dc.date2000-03-14
dc.date2000-07-27
dc.date.accessioned2026-07-07T01:52:44Z
dc.date.available2026-07-07T01:52:44Z
dc.descriptionThe paper claimed that significant radial migration of stars in a stellar disk like that of the Milky Way could not occur. We now think that while the treatment of the effects of molecular clouds was correct, the paper seriously underestimated the ability of spiral arms to shift the radii of stars that corotate with them. Consequently, it is likely that significant radial migration_is_ possible.
dc.descriptionPaper withdrawn because its principal conclusion is proably wrong
dc.identifierhttps://arxiv.org/abs/astro-ph/0003194
dc.identifierhttp://arxiv.org/abs/astro-ph/0003194
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/718
dc.subjectAstrophysics
dc.titleDisk heating and stellar migration in galaxies
dc.typetext

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