Dynamo in protostars

VERMA, MAHENDRA K ; KARAK, BIDYA BINAY ; KUMAR, ROHIT (2013) Dynamo in protostars Pramana - Journal of Physics, 81 (6). pp. 1037-1043. ISSN 0304-4289

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Official URL: http://doi.org/10.1007/s12043-013-0628-y

Related URL: http://dx.doi.org/10.1007/s12043-013-0628-y

Abstract

In this paper, we estimate the magnetic Reynolds number of a typical protostar before and after deuterium burning, and claim for the existence of dynamo process in both the phases, because the magnetic Reynolds number of the protostar far exceeds the critical magnetic Reynolds number for dynamo action. Using the equipartition of kinetic and magnetic energies, we estimate the steady-state magnetic field of the protostar to be of the order of kilogauss, which is in good agreement with observations.

Item Type:Article
Source:Copyright of this article belongs to Indian Academy of Sciences.
ID Code:118953
Deposited On:05 Jun 2021 05:24
Last Modified:05 Jun 2021 05:24

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