Standard spectroscopic methods for O-star vsini and macroturbulence only reliably measure the quantity sqrt(v_mac^2/2 + vsini^2/4) when neither clearly dominates, requiring re-analysis of prior rotation distributions.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2026 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Effects on vsini determinations of O stars from 3D model atmospheres with high turbulent velocities
Standard spectroscopic methods for O-star vsini and macroturbulence only reliably measure the quantity sqrt(v_mac^2/2 + vsini^2/4) when neither clearly dominates, requiring re-analysis of prior rotation distributions.