MACHO RR LYRAE IN THE INNER HALO AND BULGE

Capitulo de libro

Fecha

1999

Registro en:

1-886733-86-4

http://hdl.handle.net/10533/165052

1990440

http://repositorioslatinoamericanos.uchile.cl/handle/2250/1543854

Institución

ANID (Chile)

Resumen

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].

Mostrar el registro completo del ítem