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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
Affiliation:
Departamento de Física, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, RN, Brazil email: [email protected]
J. R. De Medeiros
Affiliation:
Departamento de Física, Universidade Federal do Rio Grande do Norte, 59072-970 Natal, RN, Brazil email: [email protected]
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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
Copyright
Copyright © International Astronomical Union 2013 

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