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astro-ph200872 cited

The spatial distribution of star and cluster formation in M51

R. A. Scheepmaker, H. J. G. L. M. Lamers, P. Anders +1

Aims. We study the connection between spatially resolved star formation and young star clusters across the disc of M51. Methods. We combine star cluster data based on B, V, and I-b…

astro-ph200810 cited

Spectroscopy of globular clusters in the low-luminosity spiral galaxy NGC 45

Marcelo D. Mora, Soeren S. Larsen, Markus Kissler-Patig

CONTEXT: Extragalactic globular clusters have been studied in elliptical galaxies and in a few luminous spiral galaxies, but little is known about globular clusters in low-luminosi…

astro-ph2007

A peculiar object in M51: fuzzy star cluster or a background galaxy?

R. A. Scheepmaker, H. J. G. L. M. Lamers, S. S. Larsen +1

Aims: We study a peculiar object with a projected position close to the nucleus of M51. It is unusually large for a star cluster in M51 and we therefore investigate the three most…

astro-ph2007

Resolving Extragalactic Star Clusters with HST/ACS

S. S. Larsen

With HST, colour-magnitude diagrams (CMDs) can be obtained for young star clusters well beyond the Local Group. Such data can help constrain cluster ages and metallicities, and als…

astro-ph200799 cited

ACS imaging of star clusters in M51. I. Identification and radius distribution

R. A. Scheepmaker, M. R. Haas, M. Gieles +3

We use HST/ACS observations of the spiral galaxy M51 in F435W, F555W and F814W to select a large sample of star clusters with accurate effective radius measurements in an area cove…

astro-ph2006

Variation of the cluster luminosity function across the disk of M51

M. R. Haas, M. Gieles, R. A. Scheepmaker +3

We study the luminosity function (LF) of the star clusters in M51. Comparing the observed LF with the LF resulting from artificial cluster populations suggests that there exists an…