Doppler imaging and differential rotation of Coronae Borealis using SONG
arXiv:2005.02592 · doi:10.3847/1538-4357/ab8229
Abstract
We present new Doppler images of both components of the double-lined binary CrB, based on the high-resolution spectroscopic data collected during 11 nights in 2015 March--April. The observed spectra form two independent data sets with sufficient phase coverage. We apply the least-squares deconvolution to all observed spectra to obtain high signal-to-noise mean profiles, from which we derive the Doppler images of both components of CrB simultaneously. The surfaces of both F9 and G0 components are dominated by pronounced polar spots. The F9 component exhibits a weak spot at latitude 30 and its mid-to-low latitudes are relatively featureless. The G0 star shows an extended spot structure at latitude 30, and its surface spot coverage is larger than that of the F9 star, which suggests a higher level of magnetic activity. With the cross-correlation method, we derive a solar-like surface differential rotation on the G0 star of CrB for the first time, and the surface shear rate is rad d and . We do not obtain a clear surface shear law for the F9 star due to the lack of mid-to-low latitude features, but detect a systematic longitude shift of high-latitude spots, which indicates a slower rotation with respect to the co-rotating frame.
9 figures, 2 tables, accepted for publication in ApJ
References in corpus (11)
- First Results From The Hertzsprung Song Telescope: Asteroseismology Of The G5 Subgiant Star {\Mu}Her
- The Visual Orbit of the 1.1-day Spectroscopic Binary σ^2 Coronae Borealis from Interferometry at the CHARA Array
- Differential rotation on both components of the pre main-sequence binary system HD 155555
- Conducting the SONG: The robotic nature and efficiency of a fully automated telescope
- Rotation--differential rotation relationships for late-type single and binary stars from Doppler imaging
- Anti-solar differential rotation on the active sub-giant HU Virginis
- Time-series Doppler imaging of the red giant HD 208472. Active longitudes and differential rotation
- Lithium enrichment on the single active K1-giant DI Piscium -- Possible joint origin of differential rotation and Li enrichment
- Doppler images of the eclipsing binary ER Vulpeculae
- The first Doppler imaging of the active binary prototype RS Canum Venaticorum
- Doppler images and the underlying dynamo. The case of AF Leporis