MACHO RR LYRAE IN THE INNER HALO AND BULGE
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...
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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].
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Book's title
THE THIRD STROMLO SYMPOSIUM: THE GALACTIC HALO
Publication date of the book
1999Start page
284
End page
289