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Properties of massive Population III and metal-poor stars

Published online by Cambridge University Press:  01 August 2006

Daniel Schaerer
Daniel Schaerer*
Affiliation:
Geneva Observatory, 51 Ch. des Maillettes, CH–1290 Sauverny, Switzerland email: [email protected] Laboratoire d'Astrophysique, OMP, 14 Avenue E. Belin, F-31400 Toulouse, France
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Abstract

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We review the properties of massive Population III and very metal-poor stars, including briefly their formation, IMF, their main sequence evolution, possible mass loss mechanisms, atmosphere modeling etc. For detailed predictions concerning the properties of these stars we refer to Schaerer (2002) and Schaerer (2002) and references therein. Extending these calculations, Schaerer (2007) present new calculations concerning the ionizing power, Ly-α strength and related properties for different metallicities as well as for a range of power-law and log-normal IMFs. For illustrations from these studies see the Figures below. New detailed calibrations for solar metallicity O-type stars have recently been presented by Martins et al. (2005).

Keywords

galaxies:high-redshiftstars: Population IIIstars: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 211
Copyright
Copyright © International Astronomical Union 2007

References

Martins, F., Schaerer, D., & Hillier, D. J. 2005, A&A, 436, 1049Google Scholar
Schaerer, D. 2002, A&A, 382, 28Google Scholar
Schaerer, D. 2003, A&A, 397, 527Google Scholar
Schaerer, D., & Fall, M. 2007, in preparationGoogle Scholar