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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© 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
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