Power-law statistics and stellar rotational velocities in the Pleiades

Details Power-law statistics and stellar rotational velocities in the Pleiades Power-law statistics and stellar rotational velocities in the Pleiades

2009-03-04

arxiv.org/abs/0903.0836v1

Europhys. Lett.84:59001, 2008

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

13 pages, 3 figures

Scientific paper

10.1209/0295-5075/84/59001

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 $\kappa$
and $q$-distributions with the Maxwellian.

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