M31, M33 and the Milky Way: Similarities and Differences

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dc.creatorWyse, Rosemary F. G.
dc.date2002-04-11
dc.date.accessioned2026-07-07T02:03:24Z
dc.date.available2026-07-07T02:03:24Z
dc.descriptionThe large galaxies in the Local Group, while all disk galaxies, have diverse stellar populations. A better understanding of these differences, and a physical understanding of the causes, requires more detailed study of the older populations. This presents a significant challenge to GAIA but the scientific returns are also significant.
dc.descriptionNine pages, two figures. Review for proceedings of Les Houches School May 2001, `GAIA: A European Space Project', eds O. Bienayme and C. Turon. To appear, 2002, as European Astronomical Society Pub Ser Vol 2 (Published by Edition de Physique). Style file included
dc.identifierhttps://arxiv.org/abs/astro-ph/0204190
dc.identifierhttp://arxiv.org/abs/astro-ph/0204190
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4370
dc.subjectAstrophysics
dc.titleM31, M33 and the Milky Way: Similarities and Differences
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