Near-IR spectroscopic ages of massive star clusters in M82
A. Lançon; J. S. Gallagher; M. Mouhcine; L. J. Smith; D. Ladjal; R. de Grijs · 2008 · arXiv
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Abstract (excerpt)
Like other starburst galaxies, M82 hosts compact, massive young star clusters that are interesting both in their own right and as benchmarks for population synthesis models. Can spectral synthesis models at resolutions around 1000 adequately reproduce the near-IR spectral features and the energy distribution of these clusters between 0.8 and 2.4 microns? How do the derived cluster properties compare with previous results from optical studies? We analyse the spectra of 5 massive clusters in M82, using data acquired with the spectrograph SpeX on the InfraRed Telescope Facility (NASA/IRTF) and a
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Metadata source: arXiv