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MACHO RR LYRAE IN THE INNER HALO AND BULGE

dc.creatorAlcock, C.
dc.creatorAllsman, R. A.
dc.creatorAlves, D. R.
dc.creatorBecker, Andrew C.
dc.creatorBennett, D. P.
dc.creatorCook, K. H.
dc.creatorDrake, Andrew John
dc.creatorFreeman, K. C.
dc.creatorGriest, K.
dc.creatorLehner, M. J
dc.creatorMarshall, S. L.
dc.creatorMinniti Del Barco, Dante
dc.creatorPeterson, B. A.
dc.creatorPratt, M. R.
dc.creatorQuinn, P. J.
dc.creatorRodgers, A. W.
dc.creatorStubbs, Christoper W.
dc.creatorSutherland, W.
dc.creatorTomaney, A. B.
dc.creatorVandehei, T.
dc.creatorWelch, Douglas
dc.date.accessioned2016-12-27T21:48:50Z
dc.date.available2016-12-27T21:48:50Z
dc.date.issued1999
dc.identifier.isbn1-886733-86-4 
dc.identifier.urihttp://hdl.handle.net/10533/165052
dc.description.abstractThe RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].The RR Lyrae in the bulge have been proposed to be the oldest populations in the Milky Way, tracers of how the galaxy formed. We study here the distribution of ~1600 bulge RR Lyrae stars found by the MACHO Project. The RR Lyrae with Galactocentric radius 0.4<R<3 kpc show a density law that is consistent with the extension of the metal-poor stellar halo present in the outer regions of the Milky Way. MACHO RR Lyrae in the Inner Halo and Bulge (PDF Download Available). Available from: https://www.researchgate.net/publication/234220530_MACHO_RR_Lyrae_in_the_Inner_Halo_and_Bulge [accessed Apr 21, 2016].
dc.language.isoeng
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI2.0
dc.relationinstname: Conicyt
dc.relationreponame: Repositorio Digital RI 2.0
dc.relation.ispartofseriesASP CONFERENCE SERIES
dc.titleMACHO RR LYRAE IN THE INNER HALO AND BULGE
dc.typeCapitulo de libro
dc.bibliographicCitation.stpage284
dc.bibliographicCitation.endpage289
dc.identifier.folio1990440
dc.description.conicytprogramFONDECYT
dc.relation.projectidinfo:eu-repo/grantAgreement/Fondecyt/1990440
dc.relation.setinfo:eu-repo/semantics/dataset/hdl.handle.net/10533/93479
dc.rights.driverinfo:eu-repo/semantics/openAccess
dc.type.driverinfo:eu-repo/semantics/bookPart
dc.description.shortconicytprogramFONDECYT
dc.title.libroTHE THIRD STROMLO SYMPOSIUM: THE GALACTIC HALO
dc.creator.libroAxelrod, Rim S.
dc.creator.libroGibson, Brad K.
dc.creator.libroPutman, Mary E.
dc.description.libropages515
dc.publisher.editorialAMERICAN CONCRETE INSTITUTE


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