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- W3100395361 abstract "In this paper we will show that, the non-Gaussian statistics framework based on the Kaniadakis statistics is more appropriate to fit the observed distributions of projected rotational velocity measurements of stars in the Pleiades open cluster. To this end, we compare the results from the κ and q-distributions with the Maxwellian." @default.
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- W3100395361 date "2008-12-01" @default.
- W3100395361 modified "2023-10-01" @default.
- W3100395361 title "Power law statistics and stellar rotational velocities in the Pleiades" @default.
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- W3100395361 doi "https://doi.org/10.1209/0295-5075/84/59001" @default.
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