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Expulsion of Dust from Young Stellar Clusters

Published online by Cambridge University Press:  21 March 2013

P. Grosbøl
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, D-85748 Garching, Germany email: [email protected]
H. Dottori
Affiliation:
Instituto de Física, Univ. Federal do Rio Grande do Sul, Av. Bento Gonçalves 9500, 91501-970 Porto Alegre, RS, Brazil email: [email protected]
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Abstract

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Young stellar clusters were identified on deep near-infrared images of 6 nearby, grand-design spirals observed with HAWK-I/VLT. A 90% completeness was reached for cluster complexes with MK = −11.5m (corresponding to masses around 104 M) while the linear resolution was around 40 pc. The distribution of clusters in the (H-K)–(J-H) diagrams revealed two groups of clusters. Comparing with Starburst99 model tracks, the groups could be interpreted as one old population of clusters with low extinction and one consisting of young clusters with visual extinction as high as AV = 7m. The clear separation between the two groups suggests a rapid expulsion of dust from the young clusters.

Monte-Carlo models were made assuming a cluster distribution function g(Mc, τ) = Mca τ−γ where Mc and τ are cluster mass and age, respectively. Fitting such models to the observed NIR color distributions, it was concluded that the cluster mortality had to be significant with γ = 0.8-1.0. Further, the star formation phase of clusters has to extend over several Myr. Young clusters have high extinctions at least the first 3 Myr but then lose their reddening over a period of around 5 Myr, depending on the exact evolutionary tracks used.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2013

References

Grosbøl, P. & Dottori, H. 2012, A&A, 542, A39Google Scholar
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