You are here

Uncovering a Missing Link Between Dwarf Galaxies and Globular Clusters

Content has no owner

Deep Gemini imaging of the cluster of galaxies Hydra I (also known as Abell 1060) at a distance of 54 Mpc (176 million light-years) has revealed an abundance of massive luminous metal-rich globular clusters that appears to impersonate ultra-compact dwarf galaxies. This is the richest population of such massive stellar systems ever found in any nearby galaxy clusters. This new finding by Elizabeth M. H. Wehner and William E. Harris (McMaster University, Hamilton, Canada) indicates that these massive stellar clusters may be transition objects between Ultra-Compact Dwarf (UCDs) galaxies and the more familiar massive globular clusters.

UCDs are a recently discovered type of old stellar system – too faint and compact to be called normal dwarf elliptical galaxies, but too big and bright to be called conventional globular clusters. Small numbers of them have been identified and studied in the nearby Virgo and Fornax clusters of galaxies over the past few years and have also been called “Dwarf-Globular Transition Objects.” But in the Hydra cluster the UCDs actually appear as a red and luminous extension to the sequence of most massive and metal-rich globular clusters. These UCDs appear to be closely associated with the Hydra central giant elliptical NGC 3311. Their masses are all above six million solar masses and extend to almost 30 million solar masses, making them very “high-end” globular clusters indeed – if they were forced to fit into that category. Structurally they are very compact, for comparison, dwarf galaxies have scale lengths of about 300 parsecs, while these UCDs are at least ten-times smaller and thus hard to distinguish from globular clusters other than by their exceptionally high luminosities.

The images for this study were obtained with the Gemini Multi-Object Spectrograph (GMOS) at Gemini South (Figure 1). The photometry is deep, reaching limiting magnitudes of 26.7 in the g’ band and 26.2 in the i’ band (Figure 2).

Wehner & Harris have also constructed a full-color image of the Hydra field (shown in the background box on this page), tailored to show the thousands of globular clusters around NGC 3311. This image is not in the Wehner & Harris paper but can be found at

For more details, see the article “UCD candidates in the Hydra Cluster”, by E. M. H. Wehner and W. E. Harris, in The Astrophysical Journal Letters, 2007, in press.

This deep image shows the central region of the Hydra Cluster. Galaxies include a giant elliptical (NGC 3331) in the center, another large elliptical (NGC 3309) above and right, and several faint, possible dwarf galaxy candidates (circled).

Figure 1. Deep GMOS-South image in the i’ band of the central part of the Hydra Cluster. The field is 5.5 arcminutes across. NGC 3331 is the large massive elliptical in the center, while NGC 3309, another large elliptical, is to the upper right. The circles mark the location of ultra-compact dwarf candidates. The shadow (in white) of the GMOS guide probe is seen at the bottom.

This plot shows the color and brightness of stars in the globular clusters around NGC 3311. A box highlights the location of ultra-compact dwarf (UCD) candidates.

Figure 2. This color-magnitude diagram for the globular clusters around NGC 3311 show the location (red box) of the UCD candidates or massive globular clusters.

News Archive Filter

Uncovering a Missing Link Between Dwarf Galaxies and Globular Clusters | Gemini Observatory


The website encountered an unexpected error. Please try again later.