Nazé, Y.; Broos, P. S.; Oskinova, L.; Townsley, L. K.; Cohen, D.; Corcoran, M. F.; Evans, N. R.; Gagné, M.; Moffat, A. F. J.; Pittard, J. M.; Rauw, G.; ud-Doula, A.; Walborn, N. R.
(2011)
The key empirical property of the X-ray emission from O stars is a strong correlation between the bolometric and X-ray luminosities. In the framework of the Chandra Carina Complex Project, 129 O and B stars have been ...
