Abstract
The Hyades K0 giants should all have the same age, mass, and gravity. Their UV continua therefore should be very similar. IUE data in the wavelength range 1800 - 2000 Å show, however, that their fluxes differ by large factors. Possible explanations for this phenomenon are considered.
Cite
CITATION STYLE
APA
Bohm-Vitense, E. (2008). The puzzle of the UV continua of the Hyades giants. In Cool Stars, Stellar Systems, and the Sun (pp. 273–275). Springer Berlin Heidelberg. https://doi.org/10.1007/3-540-12907-3_215
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