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Galaxy Interactions at Low and High Redshift pp 53Cite as

Total Mass and Luminosity of Star Forming Regions in the Lmc: the Predicted Infrared Fluxes

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Part of the book series: International Astronomical Union ((IAUS,volume 186))

Abstract

We have investigated 4 Shapley constellations (1996, A&A, 308, 40) to define the associated stellar complexes and their properties. From observed star counts and recent spectral classification we derive an age estimate and the upper mass limit of individual stars in these regions.

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Author information

Authors and Affiliations

  1. Astronomical Institute, National Observatory of Athens, Greece

    V. Missoulis, A. Dapergolas & E. Kontizas

  2. Department of Physics, National University of Athens, Greece

    M. Kontizas

  3. Astrophysics Group, Blackett Laboratory, Department of Physics, Imperial College, London, England

    S. Oliver

Authors
  1. V. Missoulis
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  2. A. Dapergolas
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  3. E. Kontizas
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  4. M. Kontizas
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  5. S. Oliver
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Editor information

Editors and Affiliations

  1. Institute for Astronomy, University of Hawaii, Honolulu, HI, USA

    J. E. Barnes  & D. B. Sanders  & 

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© 1999 Springer Science+Business Media Dordrecht

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Missoulis, V., Dapergolas, A., Kontizas, E., Kontizas, M., Oliver, S. (1999). Total Mass and Luminosity of Star Forming Regions in the Lmc: the Predicted Infrared Fluxes. In: Barnes, J.E., Sanders, D.B. (eds) Galaxy Interactions at Low and High Redshift. International Astronomical Union, vol 186. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4665-4_8

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  • DOI: https://doi.org/10.1007/978-94-011-4665-4_8

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-0-7923-5833-6

  • Online ISBN: 978-94-011-4665-4

  • eBook Packages: Springer Book Archive

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