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Conference object . 2021
License: CC BY
Data sources: Datacite
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Conference object . 2021
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MODELING OF 3D ATMOSPHERES OF COOL STARS WITH THE MANCHA CODE

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 26 Feb 2021 English Publisher:Zenodo
Authors: Andrea Perdomo; Elena Khomenko; N. Vitas; Manuel Collados;

doi: 10.5281/zenodo.4564016 , 10.5281/zenodo.4564017

MODELING OF 3D ATMOSPHERES OF COOL STARS WITH THE MANCHA CODE

Abstract

The first results of the application of the MANCHA code to the case of stars beyond the solar case are presented: hydrodynamical simulations of stars of spectral type K0V and M0V compared with the solar case.

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Keywords

convection, hydrodynamics, stellar atmospheres, cool stars, simulations

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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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