No SunLike Dynamo on the Active Star ζ Andromedae from Starspot Asymmetry
Sunspots are cool areas caused by strong surface magnetic fields that inhibit convection1,2. Moreover, strong magnetic fields can alter the average atmospheric structure3, degrading our ability to measure stellar masses and ages. Stars that are more active than the Sun have more and stronger dark spots than does the Sun, including on the rotational pole4. Doppler imaging, which has so far produced the most detailed images of surface structures on other stars, cannot always distinguish the hemisphere in which the starspots are located, especially in the equatorial region and if the data quality is not optimal5. This leads to problems in investigating the north–south distribution of starspot active latitudes (those latitudes with more starspot activity); this distribution is a crucial constraint of dynamo theory. Polar spots, whose existence is inferred from Doppler tomography, could plausibly be observational artefacts6. Here we report imaging of the old, magnetically active star ζ Andromedae using long-baseline infrared interferometry. In our data, a dark polar spot is seen in each of two observation epochs, whereas lower-latitude spot structures in both hemispheres do not persist between observations, revealing global starspot asymmetries. The north–south symmetry of active latitudes observed on the Sun7 is absent on ζ And, which hosts global spot patterns that cannot be produced by solar-type dynamos8.
Harmon, Robert O.; Roettenbacher, Rachel; Monnier, John; and Korhonen, H., "No SunLike Dynamo on the Active Star ζ Andromedae from Starspot Asymmetry" (2016). Physics & Astronomy Faculty Work. 2.
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