A spectro-polarimetric study of the planet-hosting G dwarf, HD 147513
A spectro-polarimetric study of the planet-hosting G dwarf, HD 147513
The results from a spectro-polarimetric study of the planet-hosting Sun-like star, HD 147513 (G5V), are presented here. Robust detections of Zeeman signatures at all observed epochs indicate a surface magnetic field, with longitudinal magnetic field strengths varying between 1.0-3.2 G. Radial velocity variations from night to night modulate on a …