Near-infra-red spectroscopic ages of massive star clusters in M 82

@article{Lanccon2008NearinfraredSA,
  title={Near-infra-red spectroscopic ages of massive star clusters in M 82},
  author={A. Lanccon and J. Gallagher and M. Mouhcine and L. Smith and D. Ladjal and R. Grijs},
  journal={Astronomy and Astrophysics},
  year={2008},
  volume={486},
  pages={165-176}
}
  • A. Lanccon, J. Gallagher, +3 authors R. Grijs
  • Published 2008
  • Physics
  • Astronomy and Astrophysics
  • Context. Like other starburst galaxies, M 82 hosts compact, massive (>5 x 10(5) M-circle dot) young star clusters that are interesting both in their own right and as benchmarks for population synthesis models. Aims. In addition to assessing or reassessing the properties of some of the brightest near-IR sources in M 82, this paper addresses the following questions. Can population synthesis models at lambda/delta lambda similar or equal to 750 adequately reproduce the near-IR spectral features… CONTINUE READING
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