Local dynamo in stars beyond the Sun: Study for a K0V star

Bibcode
2020sea..confE.206P
Perdomo García, A.; Vitas, N.; Khomenko, E.; Collados Vera, M. A.
Referencia bibliográfica

Contributions to the XIV.0 Scientific Meeting (virtual) of the Spanish Astronomical Society

Advertised on:
7
2020
Número de autores
4
Número de autores del IAC
4
Número de citas
0
Número de citas referidas
0
Descripción
We present the first results of application of the MANCHA3D code (Felipe 2010; Khomenko et al. 2017, 2018) to a K0V cool star. Initially we run the code solving purely hydrodynamic equations until the stationary convection is reached. Then we produce the magnetic field generation and amplification by Biermann's battery seed and local dynamo. We find values around 100 Gauss for the amplified saturated magnetic field, similar to those found in Khomenko et al. (2017) for the solar case.
Tipo
Sin árbitro

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