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19962023
most citedA catalogue of masses, structural parameters and velocity dispersion profiles of 112 Milky Way globular clusters

559 citations · 9.7k across the 192 of their papers we have counts for

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Showing 2007Show all

6 papers · 1 filter

astro-ph2007★ 68 cited

The dark matter halo of NGC 1399 - CDM or MOND?

T. Richtler, Y. Schuberth, M. Hilker +3

Central galaxies in galaxy clusters may be key discriminants in the competition between the cold dark matter (CDM) paradigm and modified Newtonian dynamics (MOND). We investigate t…

astro-ph2007

Stroemgren metallicity calibration: the m1, b-y relation

A. Calamida, G. Bono, P. B. Stetson +15

We performed a new calibration of the Stroemgren metallicity index m1 based on the b-y color of cluster red giant stars. The current Metallicity-Index-Color relation is not linear…

astro-ph2007★ 1 cited

A flat faint end of the Fornax cluster galaxy luminosity function

Steffen Mieske, Michael Hilker, Leopoldo Infante +1

We analyse the photometric properties of the early-type Fornax cluster dwarf galaxy population (M_V>-17 mag), based on a wide field imaging study of the central cluster area in V a…

astro-ph2007★ 73 cited

Stroemgren photometry of Galactic Globular Clusters. I. New Calibrations of the metallicity index

A. Calamida, G. Bono, P. B. Stetson +15

We present a new calibration of the Stroemgren metallicity index m1 using red giant (RG) stars in 4 globular clusters (GCs:M92,M13,NGC1851,47Tuc) with metallicity ranging from [Fe/…

astro-ph2007★ 57 cited

A search for ultra-compact dwarf galaxies in the Centaurus galaxy cluster

S. Mieske, M. Hilker, A. Jordan +2

Aim: To extend the investigations of ultra-compact dwarf galaxies (UCDs) beyond the well studied Fornax and Virgo clusters. Methods: We measured spectroscopic redshifts of about 40…

astro-ph2007

Metallicity distribution of Omega Cen Red Giants based on the Stroemgren m1 metallicity index

A. Calamida, G. Bono, L. M. Freyhammer +6

We adopted uvby Stroemgren photometry to investigate the metallicity distribution of Omega Cen Red Giant (RG) stars. We provided a new empirical calibration of the Stroemgren m1 =…