The IACOB project. II. On the scatter of O-dwarf spectral type - effective temperature calibrations
Context. We are now in an era of large spectroscopic surveys of OB-type stars. Quantitative spectroscopic analysis of these modern datasets is enabling us to review the physical properties of blue massive stars with robust samples, not only revisiting mean properties and general trends, but also incorporating information about the effects of second
Simón-Díaz, S. et al.
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2014