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Variations in the width, density, and direction of the Palomar 5 tidal tails
(IOP, 2020)
Stars that escape globular clusters form tidal tails that are predominantly shaped by the global distribution of mass in the Galaxy, but also preserve a historical record of small-scale perturbations. Using deep grz ...
The Origin of the Milky Way's Halo Age Distribution
(2018)
We present an analysis of the radial age gradients for the stellar halos of five Milky Way (MW) mass-sized systems simulated as part of the Aquarius Project. The halos show a diversity of age trends, reflecting their ...
MACHO RR LYRAE IN THE INNER HALO AND BULGE
(AMERICAN CONCRETE INSTITUTE, 1999)
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 ...
MACHO RR LYRAE IN THE INNER HALO AND BULGETHE THIRD STROMLO SYMPOSIUM: THE GALACTIC HALO
(AMERICAN CONCRETE INSTITUTE, 2016)
THE MILKY WAY, OUR GALAXYLa Vía Láctea, nuestra galaxia
(Facultad de Ciencias, 2010)
THE MILKY WAY, OUR GALAXYLa Vía Láctea, nuestra galaxia
(Facultad de Ciencias, 2010)
Discovery of extended tidal tails around the globular cluster Palomar 13
(The American Astronomical Society, 2020)
We use photometry from the DECam Legacy Survey to detect candidate tidal tails extending ∼5° on either side of the Palomar 13 globular cluster. The tails are aligned with the proper motion of Palomar 13 and are consistent ...
The cold veil of the milky way stellar halo
(OXFORD UNIV PRESS, 2012)