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Resolved and unresolved populations: statistics and synthesis models

Published online by Cambridge University Press:  26 May 2016

Miguel Cerviño
Miguel Cerviño*
Affiliation:
ESA Laboratorio de Astrofísica Espacial y Física Fundamental (INTA), Apdo. 50727, E-28080 Madrid, España, and Instituto de Astrofísica de Andalucía (CSIC), Camino Bajo de Huétor 24, E-18080 Granada, España

Abstract

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In this contribution, I present 90%-confidence limits on diagnostic diagrams of Wλ(WR-bump) and L(WR-bump)/L(Hβ) ratio vs.Wλ(Hβ) resulting from evolutionary synthesis models that include the statistical dispersion due to finite stellar populations in real star forming regions.

Type
Part 3. Location and Distribution of Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 545 - 546
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Cerviño, M., Valls-Gabaud, D., Luridiana, V., Mas-Hesse, J.M. 2002, A&A 381, 51.Google Scholar