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Properties of the O-type giants and supergiants in 30 Doradus

Published online by Cambridge University Press:  28 July 2017

O. H. Ramírez-Agudelo
Affiliation:
UK ATC, Royal Observatory Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK email: oscar.ramirez@stfc.ac.uk
VFTS consortium
Affiliation:
UK ATC, Royal Observatory Edinburgh, Blackford Hill, Edinburgh, EH9 3HJ, UK email: oscar.ramirez@stfc.ac.uk
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Abstract

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We discuss the stellar and wind properties of 72 presumably single O-type giants, bright giants, and supergiants in the 30 Doradus region. This sample constitutes the largest and most homogeneous sample of such stars ever analyzed and offers the opportunity to test models describing their main-sequence evolution.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

Evans, et al., 2011, A&A, 530, A108 Google Scholar
Ramírez-Agudelo, et al., 2017, A&A, 600, A81 Google Scholar