activity
20062009
most citedAn extreme IMF as an explanation for high M/L ratios in UCDs? The CO index as a tracer of bottom heavy IMFs

76 citations · 298 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO200972 cited

The early-type dwarf galaxy population of the Centaurus cluster

I. Misgeld, M. Hilker, S. Mieske

We present a photometric study of the early-type dwarf galaxy population of the Centaurus cluster, aiming at investigating the galaxy luminosity function (LF) and galaxy scaling re…

astro-ph200862 cited

High mass-to-light ratios of UCDs - Evidence for dark matter ?

Holger Baumgardt, Steffen Mieske

Ultra-compact dwarf galaxies (UCDs) are stellar systems with masses of around 10^7 to 10^8 Msun and half mass radii of 10-100 pc. They have some properties in common with massive g…

astro-ph200815 cited

Compact stellar systems in the Fornax cluster: a UV perspective

Steffen Mieske, Michael Hilker, Dominik J. Bomans +4

In recent years, increasing evidence for chemical complexity and multiple stellar populations in massive globular clusters (GCs) has emerged, including extreme horizontal branches…

astro-ph200776 cited

An extreme IMF as an explanation for high M/L ratios in UCDs? The CO index as a tracer of bottom heavy IMFs

Steffen Mieske, Pavel Kroupa

A new type of compact stellar systems, labelled ``ultra-compact dwarf galaxies'' (UCDs), was discovered in the last decade. Recent studies show that their dynamical mass-to-light r…

astro-ph200716 cited

On the efficiency of field star capture by star clusters

Steffen Mieske, Holger Baumgardt

An exciting recent finding regarding scaling relations among globular clusters is the so-called 'blue tilt': clusters of the blue sub-population follow a trend of redder colour wit…

astro-ph200757 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…