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Stochasticity effects on derivation of physical parameters of unresolved star clusters

We developed a method for a fast modeling of broad-band UBVRI integrated magnitudes of unresolved star clusters and used it to derive their physical parameters (age, mass, and extinction). The method was applied on M33 galaxy cluster sample and consistency of ages and masses derived from unresolved observations with the values derived from resolved stellar photometry was demonstrated. We found that interstellar extinction causes minor age-extinction degeneracy for the studied sample due to a narrow extinction range in M33.

preprint2013arXivOpen access
Philippe de MeulenaerDonatas NarbutisTadas MineikisVladas Vansevičius
astro-ph.GA
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Open access4 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
Citations: 0Reviews: 0Saves: 0Code: not linkedDataset: not linkedInstitutions: 0

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Philippe de MeulenaerDonatas NarbutisTadas MineikisVladas Vansevičius

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