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19942023
most citedAge and Metallicity Distribution of the Galactic Bulge from Extensive Optical and Near-IR Stellar Photometry

449 citations · 4.4k across the 88 of their papers we have counts for

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Showing 1999Show all

8 papers · 1 filter

astro-ph1999

Stellar yields and chemical evolution - The solar neighborhood as a calibrator

Daniel Thomas, Laura Greggio, Ralf Bender

Uncertainties in stellar nucleosynthesis and their impact on models of chemical evolution are discussed. Comparing the Type II supernova nucleosynthesis prescriptions from Woosley…

astro-ph1999★ 27 cited

A Near-Infrared Stellar Census of the Blue Compact Dwarf Galaxy VII~Zw~403

Regina E. Schulte-Ladbeck, Ulrich Hopp, Laura Greggio +1

We present near-infrared single-star photometry for the low-metallicity Blue Compact Dwarf galaxy VII~Zw~403. We achieve limiting magnitudes of F110W~~25.5 and F160W~$\app…

astro-ph1999★ 18 cited

The uncertainties in the synthetic indices for stellar populations

Claudia Maraston, Laura Greggio, Daniel Thomas

The study of line strengths in the spectra of early-type galaxies has proven to be a powerful tool for investigating the age and the metallicity of these systems. When computing mo…

astro-ph1999★ 40 cited

A Stellar Population Gradient in VII Zw 403 - Implications for the Formation of Blue Compact Dwarf Galaxies

Regina E. Schulte-Ladbeck, Ulrich Hopp, Mary M. Crone +1

We present evidence for the existence of an old stellar halo in the Blue Compact Dwarf galaxy VII Zw 403. VII Zw 403 is the first Blue Compact Dwarf galaxy for which a clear spatia…

astro-ph1999★ 125 cited

The Star Formation History of IZw18

A. Aloisi, M. Tosi, L. Greggio

The star formation history in IZw18 has been inferred from HST/WFPC2 archival data. This is done by comparing the derived V, B-V and V, V-I color-magnitude diagrams and luminosity…

astro-ph1999★ 6 cited

Probing early-type galaxy evolution with the Kormendy relation

B. L. Ziegler, R. P. Saglia, R. Bender +3

We investigate the evolution of early-type galaxies in four clusters at z=0.4 (Abell370, Cl0303+17, Cl0939+47 and Cl1447+26) and in one at z=0.55 (Cl0016+16). The galaxies are sele…