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MACHO RR LYRAE IN THE INNER HALO AND BULGE

Type
Capitulo de libro
Program
Programa FONDECYT
Conicyt Instrument
Proyectos Regulares
Author
Alcock, C.
Allsman, R. A.
Alves, D. R.
Becker, Andrew C.
Bennett, D. P.
Cook, K. H.
Drake, Andrew John
Freeman, K. C.
Griest, K.
Lehner, M. J
Marshall, S. L.
Minniti Del Barco, Dante
Peterson, B. A.
Pratt, M. R.
Quinn, P. J.
Rodgers, A. W.
Stubbs, Christoper W.
Sutherland, W.
Tomaney, A. B.
Vandehei, T.
Welch, Douglas
Abstract
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 (PD...   Ver más
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].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].   Ver menos
Project Id
1990440
Contest
Concurso Nacional Regular 1999
Book's title
THE THIRD STROMLO SYMPOSIUM: THE GALACTIC HALO
Publication date of the book
1999
Start page
284
End page
289
Metadata
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ANID Agencia Nacional de Investigación y Desarrollo

Moneda 1375, Santiago de Chile. Teléfono (+56 2) 365 44 00

¿NECESITAS AYUDA?

Centro de ayuda OIRS

o llámanos directamente al

(+56 2) 365 44 00

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