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The young star cluster system of the Antennae galaxies

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 22 Sep 2009Embargo end date: 01 Jan 2008 Netherlands English Publisher:Springer Science and Business Media LLCJournal:Astrophysics and Space Science, volume 324, pages 305-308 (issn: 0004-640X, eissn: 1572-946X, Copyright policy )
Authors: Peter Anders; Richard de Grijs; Richard de Grijs; Uta Fritze;

doi: 10.1007/s10509-009-0103-x , 10.48550/arxiv.0801.3679

arXiv: http://arxiv.org/abs/0801.3679

The young star cluster system of the Antennae galaxies

Abstract

The study of young star cluster (YSC) systems, preferentially in starburst and merging galaxies, has seen great interest in the recent past, as it provides important input to models of star formation. However, even some basic properties (like the luminosity function [LF]) of YSC systems are still under debate. Here we study the photometric properties of the YSC system in the nearest major merger system, the Antennae galaxies. We find evidence for the existence of a statistically significant turnover in the LF.

4 pages, 3 figures, to appear in "Young Massive Star Clusters - Initial Conditions and Environments", 2008, Astrophysics & Space Science, eds. E. Perez, R. de Grijs, R. M. Gonzalez Delgado

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Netherlands
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Keywords

Space and Planetary Science, Astrophysics (astro-ph), FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
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Average
Average
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