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most citedComplexity on Small Scales III: Iron and alpha Element Abundances in the Carina Dwarf Spheroidal Galaxy

165 citations · 449 across the 7 of their papers we have counts for

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astro-ph2008165 cited

Complexity on Small Scales III: Iron and alpha Element Abundances in the Carina Dwarf Spheroidal Galaxy

A. Koch, E. K. Grebel, G. F. Gilmore +5

We have obtained high-resolution spectroscopy of ten red giants in the Carina dwarf spheroidal (dSph) with UVES at the ESO/VLT. Here we present the abundances of O,Na,Mg,Si,Ca,Ti a…

astro-ph200769 cited

Star-formation in the HI bridge between M81 and M82

Duilia F. de Mello, L. J. Smith, E. Sabbi +3

We present multi-wavelength observations of stellar features in the HI tidal bridge connecting M81 and M82 in the region called Arp's Loop. We identify eight young star-forming reg…

astro-ph2007130 cited

Stellar kinematics in the remote Leo II dwarf spheroidal galaxy -- Another brick in the wall

A. Koch, J. T. Kleyna, M. I. Wilkinson +5

We present the projected velocity dispersion profile for the remote (d=233kpc) Galactic dwarf spheroidal (dSph) galaxy Leo II, based on 171 discrete stellar radial velocities that…

astro-ph200684 cited

Complexity on Small Scales II: Metallicities and Ages in the Leo II Dwarf Spheroidal Galaxy

A. Koch, E. K. Grebel, J. T. Kleyna +5

We present metallicities and ages for 52 red giants in the remote Galactic dwarf spheroidal (dSph) galaxy Leo II. These stars cover the entire surface area of Leo II and are radial…

astro-ph20061 cited

The Age-Metallicity Relation of the SMC

A. Kayser, E. K. Grebel, D. R. Harbeck +4

The Small Magellanic Cloud (SMC) is the only dwarf galaxy in the Local Group known to have formed and preserved populous star clusters continuously over the past 12 Gyr. These clus…

astro-ph2005

Complexity on Small Scales: The Metallicity Distribution of the Carina Dwarf Spheroidal Galaxy

A. Koch, E. K. Grebel, R. F. G. Wyse +5

The Carina dwarf spheroidal (dSph) galaxy is the only galaxy of this type that shows clearly episodic star formation separated by long pauses. Here we present metallicities for 437…