output
19932026
most citedObservational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

19.6k citations

Showing 2009 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2009★ 140 cited

Boo-1137 - An Extremely Metal-Poor Star in the Ultra-Faint Dwarf Spheroidal Galaxy Boötes I

John E. Norris, David Yong, Gerard Gilmore +1

We present high-resolution, high-S/N spectra of an extremely metal- poor giant star Boo-1137 in the "ultra-faint" dwarf spheroidal galaxy (dSph) Bootes I (absolute magnitude Mv ~ -…

astro-ph.GA2009★ 13 cited

Stellar Over-densities in the Outer Halo of the Milky Way

Stefan C. Keller

This study presents a tomographic survey of a subset of the outer halo (10-40 kpc) drawn from the Sloan Digital Sky Survey Data Release 6. Halo substructure on spatial scales of $>…

astro-ph.GA2009★ 143 cited

M22: A [Fe/H] Abundance Range Revealed

G. S. Da Costa, E. V. Held, I. Saviane +1

Intermediate resolution spectra at the Ca II triplet have been obtained for 55 candidate red giants in the field of the globular cluster M22 with the VLT/FORS instrument. Spectra w…

astro-ph.GA2009★ 141 cited

Is the Milky Way ringing? The hunt for high velocity streams

I. Minchev, A. C. Quillen, M. Williams +4

We perform numerical simulations of a stellar galactic disk with initial conditions chosen to represent an unrelaxed population which might have been left following a merger. Stars…

astro-ph.GA2009★ 60 cited

Scl-dE1 GC1: An Extended Globular Cluster in a Low-Luminosity Dwarf Elliptical Galaxy

G. S. Da Costa, E. K. Grebel, H. Jerjen +2

We report the discovery from Hubble Space Telescope ACS images of an extended globular cluster, denoted by Scl-dE1 GC1, in the Sculptor Group dwarf Elliptical galaxy Scl-dE1 (Sc22)…

astro-ph.GA2009★ 54 cited

The Chemical Evolution of Globular Clusters I. Reactive Elements and Non-Metals

Andrea Marcolini, Brad K. Gibson, Amanda I. Karakas +1

We propose a new chemical evolution model aimed at explaining the chemical properties of globular clusters (GC) stars. Our model depends upon the existence of (i) a peculiar pre-en…