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- W2963013012 abstract "Aims. Rotational speed is an important physical parameter of stars, and knowing the distribution of stellar rotational velocities is essential for understanding stellar evolution. However, rotational speed cannot be measured directly and is instead the convolution between the rotational speed and the sine of the inclination angle v sin i." @default.
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- W2963013012 date "2014-05-01" @default.
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- W2963013012 title "A method to deconvolve stellar rotational velocities" @default.
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