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• W2098276472 abstract "Context.The rotation-activity connection explains stellar activity in terms of rotation and convective overturn time. It is well established in stars of spectral types F–K as well as in M-type stars of young clusters, in which rotation is still very rapid even among M-dwarfs. The rotation-activity connection is not established in field M-dwarfs, because they rotate very slowly, and detecting rotation periods or rotational line broadening is a challenge. In field M-dwarfs, saturation sets in below vrot = 5 km s-1, hence they are expected to populate the non-saturated part of the rotation-activity connection." @default.
• W2098276472 created "2016-06-24" @default.
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• W2098276472 date "2007-02-27" @default.
• W2098276472 modified "2023-09-25" @default.
• W2098276472 title "The narrowest M-dwarf line profiles and the rotation-activity connection at very slow rotation" @default.
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• W2098276472 doi "https://doi.org/10.1051/0004-6361:20066991" @default.
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