• Corpus ID: 118427221

NGC 2362: The Terminus of Star Formation

@article{Dahm2008NGC2T,
  title={NGC 2362: The Terminus of Star Formation},
  author={Scott E. Dahm},
  journal={arXiv: Astrophysics},
  year={2008}
}
  • S. Dahm
  • Published 28 August 2008
  • Physics
  • arXiv: Astrophysics
NGC 2362 is a richly populated Galactic cluster, devoid of natal molecular gas and dust. The cluster represents the final product of the star forming process and hosts an unobscured and near-complete initial mass function. NGC 2362 is dominated by the O9 Ib multiple star, tau CMa, as well as several dozen unevolved B-type stars. Distributed throughout the cluster are several hundred suspected intermediate and low-mass pre-main sequence members. Various post-main sequence evolutionary models… 

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SGG acknowledges support from the Science & Technology Facilities Council (STFC) via an Ernest Rutherford Fellowship [ST/J003255/1]. CLD acknowledges support from STFC via a PhD studentship and

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