Stellar Spottedness Models

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R.E. Gershberg ^{1 ,*}

1 . Crimean Astrophysical Observatory, Nauchny, Crimea, Russia 298409

* Authors to whom correspondence should be addressed.

Published in Journal of Fundamental and Observational Physics and Astrophysics ( Volume 1, Issue 2 )

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Abstract

Starspots are one of the most important characteristics of stars with solar-type activity. This paper briefly outlines the history of studying these structures, from a single round spot in the middle of the past century to the present-day three-component stellar surface consisting of the quiet photosphere, cold spots, and hot faculae. Particular attention is given to the zonal spottedness model proposed and developed in Crimea, which is practically unknown to our foreign colleagues due to the fact that almost all the studies on this model have been published in Russian.

Published in	Journal of Fundamental and Observational Physics and Astrophysics (Volume 1, Issue 2)
DOI	10.65736/jfopa01023
Page(s)	9
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s). Published by Open Access Press

Keywords

flare stars, solar-type activity, starspots, zonal spottedness model

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APA Style

Gershberg, R. R. (2024). Stellar Spottedness Models. Journal of Fundamental and Observational Physics and Astrophysics, 1, (2), 3. https://doi.org/10.65736/jfopa01023

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ACS Style

Gershberg, R. Stellar Spottedness Models. Mach. Learn. Res. (2024), 1, (2), 3. doi: https://doi.org/10.65736/jfopa01023

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AMA Style

Gershberg . Stellar Spottedness Models. Mach Learn Res. (2024);1(2):3. doi: https://doi.org/10.65736/jfopa01023

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