Polarization due to rotational distortion in the bright star Regulus
arXiv:1804.06576 · doi:10.1038/s41550-017-0238-6
Abstract
Polarization in stars was first predicted by Chandrasekhar [1] who calculated a substantial linear polarization at the stellar limb for a pure electron-scattering atmosphere. This polarization will average to zero when integrated over a spherical star but could be detected if the symmetry is broken, for example by the eclipse of a binary companion. Nearly 50 years ago, Harrington and Collins [2] modeled another way of breaking the symmetry and producing net polarization - the distortion of a rapidly rotating hot star. Here we report the first detection of this effect. Observations of the linear polarization of Regulus, with two different high-precision polarimeters, range from +42 parts-per-million (ppm) at a wavelength of 741 nm to -22 ppm at 395 nm. The reversal from red to blue is a distinctive feature of rotation-induced polarization. Using a new set of models for the polarization of rapidly rotating stars we find that Regulus is rotating at 96.5% of its critical angular velocity for breakup, and has an inclination greater than 76.5 degrees. The rotation axis of the star is at a position angle of 79.50.7 degrees. The conclusions are independent of, but in good agreement with, the results of previously published interferometric observations of Regulus [3]. The accurate measurement of rotation in early-type stars is important for understanding their stellar environments [4], and course of their evolution [5].
arXiv commentThis is the full published article including the Methods and Supplementary Information sections: 33 pages, 10 figures, 8 tables
References in corpus (13)
- Validation of the new Hipparcos reduction
- Be-star rotation: how close to critical?
- Gravity darkening in rotating stars
- Rotational velocities of A-type stars IV. Evolution of rotational velocities
- First Results from the CHARA Array. I. An Interferometric and Spectroscopic Study of the Fast Rotator alpha Leonis (Regulus)
- Colder and Hotter: Interferometric imaging of β Cassiopeiae and α Leonis
- New limb-darkening coefficients and synthetic photometry for model-atmosphere grids at Galactic, LMC, and SMC abundances
- A high-sensitivity polarimeter using a ferro-electric liquid crystal modulator
- Polarization measurements of hot dust stars and the local interstellar medium
- The linear polarisation of southern bright stars measured at the parts-per-million level
- A High Precision, Optical Polarimeter to Measure Inclinations of High Mass X-Ray Binaries
- The intrinsic and interstellar broadband linear polarization of nearby FGK dwarfs
- Rapid rotators revisited: absolute dimensions of KOI-13
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