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The Cluster Birthline and the formation of stellar clusters in M33

We present a new method to analyze the IMF at its high mass end in young stellar clusters, which rely on two integrated observables: the cluster bolometric and Halpha luminosity. Using several cluster samples selected in M33 we show that a stochastically sampled universal IMF is in better agreement with the data than a truncated IMF whose maximum stellar mass depends on cluster mass. We also discuss the possibility that a delayed formation of massive stars is taking place in low density star forming regions as an alternative to a strong leakage of ionizing photons from HII regions of young luminous clusters.

preprint2010arXivOpen access
Edvige CorbelliCarlo GiovanardiMarco Grossi
astro-ph.CO
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Open access3 authors1 topic
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Edvige CorbelliCarlo GiovanardiMarco Grossi

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