Chris Flynn : Tuorla Observatory

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gold

Production of Helium. The plot shows how the luminosity of K dwarfs increases as the amount of Helium and heaver elements increases. The data points represent real K dwarf stars observed with the Hipparcos satellite. Three computer calculations are shown by the dark blue, light blue and green lines: they represent different amounts of Helium produced in stars relative to the amount of heavier metals. The data indicate that the amount of Helium produced has been twice the amount of all the heavier than Helium elements combined (purple line).
 





For further information:  

Chris Flynn
Tuorla Observatory
Väisäläntie 20
FIN-21500 Piikkiö
Finland

Tel: +358 (0)2 2744244
Fax: +358 (0)2 2433767
email: cflynn@astro.utu.fi





Antares

Research supported by the ANTARES program of the Academy of Finland