No Sun-like dynamo on the active star $\zeta$ Andromedae from starspot asymmetry
Rachael M. Roettenbacher (1), John D. Monnier (1), Heidi Korhonen, (2,3), Alicia N. Aarnio (1), Fabien Baron (1,4), Xiao Che (1), Robert O., Harmon (5), Zsolt Kovari (6), Stefan Kraus (1,7), Gail H. Schaefer (8),, Guillermo Torres (9), Ming Zhao (1,10)

TL;DR
This study uses infrared interferometry to image starspots on $$ Andromedae, revealing persistent polar spots and asymmetrical active latitudes, challenging the solar-type dynamo model for active stars.
Contribution
First direct interferometric imaging of starspots on $$ Andromedae showing persistent polar spots and asymmetrical spot distribution, questioning the applicability of solar dynamo models.
Findings
Persistent polar spots observed in two epochs.
Global starspot asymmetries inconsistent with solar-type dynamos.
Absence of north-south symmetry in starspot distribution.
Abstract
Sunspots are cool areas caused by strong surface magnetic fields inhibiting convection. Moreover, strong magnetic fields can alter the average atmospheric structure, degrading our ability to measure stellar masses and ages. Stars more active than the Sun have more and stronger dark spots than in the solar case, including on the rotational pole itself. Doppler imaging, which has so far produced the most detailed images of surface structures on other stars than the Sun, cannot always distinguish the hemisphere in which the starspots are located, especially in the equatorial region and if the data quality is not optimal. This leads to problems in investigating the north-south distribution of starspot active latitudes (those latitudes with more spot activity), which are crucial constraints of dynamo theory. Polar spots, inferred only from Doppler tomography, could plausibly be observational…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
