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Flash stars in stellar aggregates

Published online by Cambridge University Press:  14 August 2015

Guillermo Haro
Guillermo Haro*
Affiliation:
Tonantzintla and Tacubaya Observatories

Extract

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In the past 10 years numerous extremely rapid variables have been found in different stellar associations. The spectrophotometric characteristics of some of these explosive variables are so similar to those of the UV Ceti stars that we propose the term “flash stars” for this variety, in order to provisionally distinguish them from the classical flare stars.

Type
Section 1: The Galaxy
Information
Symposium - International Astronomical Union , Volume 20: The Galaxy and the Magellanic Clouds , 1964 , pp. 30 - 37
Copyright
Copyright © Australian Academy of Science 1964 

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