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- W4300610193 abstract "I discuss EINSTEIN X-ray observations of late-type (G and K) stars. For the RS CVn systems and the evolved G stars, there is a linear relation between X-ray surface flux and stellar angular velocity. The situation is more complex among the G-K dwarfs: rapid rotators, with rotational periods less than ∼10 d , also show a linear relation between X-ray surface flux and angular velocity, but the slow rotators fall some two orders of magnitude below that relation." @default.
- W4300610193 created "2022-10-03" @default.
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- W4300610193 date "1983-01-01" @default.
- W4300610193 modified "2023-10-18" @default.
- W4300610193 title "The Coronal Rotation-Activity Relations in Late-Type Stars" @default.
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- W4300610193 doi "https://doi.org/10.1017/s0074180900029855" @default.
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