{ "id": "2303.16051", "version": "v1", "published": "2023-03-28T15:33:30.000Z", "updated": "2023-03-28T15:33:30.000Z", "title": "The connection between starspots and superflares: a case study of two stars", "authors": [ "Alexandre Araújo", "Adriana Valio" ], "comment": "5 pages,4 Figures", "doi": "10.1093/mnrasl/slad034", "categories": [ "astro-ph.SR", "astro-ph.EP" ], "abstract": "How do the characteristics of starspots influence the triggering of stellar flares? Here we investigate the activity of two K-type stars, similar in every way from mass to rotation periods and planetary systems. Both stars exhibit about a hundred spots, however, Kepler-411 produced 65 superflares, while Kepler-210 presented none. The spots of both stars were characterized using the planetary transit mapping technique, which yields the intensity, temperature, and radius of starspots. The average radius was $(17\\pm7) \\times 10^3$ km and $(58 \\pm 23) \\times 10^3$ km, while the intensity ratio with respect to the photosphere was $(0.35\\pm0.24)$ $I_{c}$ and $(0.64\\pm0.15)$ $I_{c}$, and the temperature was $(3800 \\pm 700)$ K and $(4180 \\pm 240)$ K for spots of Kepler-411 and Kepler-210, respectively. Therefore, spots on the star with no superflares, Kepler-210, are mostly larger, less dark, and warmer than those on the flaring star, Kepler-411. This may indicate magnetic fields with smaller magnitude and complexity of the spots on Kepler-210 when compared to those on Kepler-411. Thus, starspot area appears not to be the main culprit of superflares triggering. Perhaps the magnetic complexity of active regions is more important.", "revisions": [ { "version": "v1", "updated": "2023-03-28T15:33:30.000Z" } ], "analyses": { "keywords": [ "case study", "superflares", "connection", "starspot area appears", "planetary transit mapping technique" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable" } } }