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A Theoretical Domain for Flare Stars in the H–R Diagram

Nature volume 202, pages 1319–1321 (1964)Cite this article

Abstract

IT has been suggested several times1 that the flare activity observed in flash and U V Ceti stars is of a nature similar to that of solar flares. In this communication I shall adhere to this point of view, which, together with present ideas about the Helmholtz–Kelvin phases of stellar evolution, will permit us to understand, in a simple manner, a number of observations regarding flares in stars.

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Authors and Affiliations

  1. Observatorio Astronómico, Universidad Nacional de Mexico, Observatorio Astrofísico de Tonantzintla, Mexico

    ARCADIO POVEDA

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  1. ARCADIO POVEDA
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POVEDA, A. A Theoretical Domain for Flare Stars in the H–R Diagram. Nature 202, 1319–1321 (1964). https://doi.org/10.1038/2021319b0

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