Chris Flynn : Tuorla Observatory

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gold

 
The Goldilocks effect. The plot shows nearby stars measured with the Hipparcos satellite, arranged from hot to cool (right to left) and very bright to very dim (up to down). "Hot stars" are too young, to be useful : they tell us little about the history of Helium production. The "Evolved stars" have been producing lots of Helium --- making them of little use as fossil records of the Helium in the Universe at the time such stars were born. Very cool stars (lower right) have very complex spectra making the prediction of their brightness still too difficult to be reliable. The K dwarfs utilised in this study are neither too cool, nor too hot, but "just right".
 





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