Determination of Vega's rotational velocity based on the Fourier analysis of spectral line profiles
Yoichi Takeda

TL;DR
This study accurately determines Vega's intrinsic rotational velocity and inclination by analyzing the Fourier transforms of spectral lines, resolving previous uncertainties about its rapid rotation viewed nearly pole-on.
Contribution
It introduces a novel method using the first zero of Fourier-transformed spectral lines to separately determine Vega's v_e and vsini, improving upon traditional profile comparison techniques.
Findings
Vega's vsini = 21.6 km/s with 0.3 km/s uncertainty
Vega's v_e = 195 km/s with 15 km/s uncertainty
Inclination angle i = 6.4 degrees with 0.5 degrees uncertainty
Abstract
While it is known that the sharp-line star Vega (vsini ~ 20km/s) is actually a rapid rotator seen nearly pole-on with low i (< 10 deg), no consensus has yet been accomplished regarding its intrinsic rotational velocity (v_e), for which rather different values have been reported so far. Methodologically, detailed analysis of spectral line profiles is useful for this purpose, since they reflect more or less the v_e-dependent gravitational darkening effect. However, direct comparison of observed and theoretically simulated line profiles is not necessarily effective in practice, where the solution is sensitively affected by various conditions and the scope for combining many lines is lacking. In this study, determination of Vega's v_e was attempted based on an alternative approach making use of the first zero (q_1) of the Fourier transform of each line profile, which depends upon K…
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