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A nonextensive approach for the angular momentum loss rate in low-mass stars

Published online by Cambridge University Press:  18 July 2013

Daniel B. de Freitas  and
J. R. De Medeiros
Daniel B. de Freitas
Affiliation:
Departamento de Física, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, RN, Brazil email: danielbrito@dfte.ufrn.br
J. R. De Medeiros
Affiliation:
Departamento de Física, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, RN, Brazil email: danielbrito@dfte.ufrn.br
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Abstract

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The present study demonstrates that behavior of rotational velocity as a function of stellar age is consistent using Tsallis' nonextensive formalism, resulting in a new approach to understanding the stellar rotational scenario.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 197 - 198
Copyright
Copyright © International Astronomical Union 2013 

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