Effective Temperatures and Gravities for O-type Stars Determined from High Precision Line Profiles and Wind-Blanketed Model Atmospheres [chapter]

B. Bohannan, S. A. Voels, D. C. Abbott, D. G. Hummer
1988 The Impact of Very High S/N Spectroscopy on Stellar Physics  
doi:10.1007/978-94-009-2937-1_23 fatcat:r46y3nsqynawbnnf4uqqmwqiqe