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- W1485042685 abstract "Disk integration of solar intensity profiles suggests that rotation enhances intermediate strength line asymmetries up to v sin i of about 6 km/s, after which the slope of the line bisector remains constant. Observed stellar line profiles do not show such a simple relation. Fast rotators exhibit large variations, owing presumably to stellar activity. Caution is advised with respect to the use of slow rotating or inactive star line profiles to determine the broadening of faster rotators." @default.
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- W1485042685 date "1990-01-01" @default.
- W1485042685 modified "2023-09-26" @default.
- W1485042685 title "Rotational enhancement of line asymmetries in F9-G2 dwarfs" @default.
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