Coronal and chromospheric emission in A-type stars
arXiv:2205.05815 · doi:10.3847/1538-3881/ac6ef6
Abstract
Cool stars on the main sequence generate X-rays from coronal activity, powered by a convective dynamo. With increasing temperature, the convective envelope becomes smaller and X-ray emission fainter. We present Chandra/HRC-I observations of four single stars with early A spectral types. Only the coolest star of this sample, Eri ( K), is detected with while the three hotter stars ( K), namely Leo, Leo, and Cen, remain undetected with upper limits . The drop in X-ray emission thus occurs in a narrow range of effective temperatures around K and matches the drop of activity in the C III and O VI transition region lines.
11 pages, 3 figures, accepted by AJ
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