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The effect of the adiabatic assumption on asteroseismic scaling relations for luminous red giants
Although stellar radii from asteroseismic scaling relations agree at the per cent level with independent estimates for main sequence and most first-ascent red giant branch (RGB) stars, the scaling relations over-predict radii at the tens of per cent level for the most luminous stars (|$R \gtrsim 30 \, \mathrm{R}_{\odot }$|). These evolved stars have significantly superadiabatic envelopes, and the extent of these regions increase with increasing radius.
Preliminary Investigation of a Novel 18F Radiopharmaceutical for Imaging CB2 Receptors in a SOD Mouse Model
RESEARCH ARTICLE (Open Access) Previous Next Contents Vol 74(6) Giancarlo Pascali A B C E , Daniele Panetta C , Mariarosaria De Simone C D , Silvia Burchielli C , Valentina Lucchesi D , Elena Sanguinetti C , Simone Zanoni B , Patricia Iozzo C , Giuseppe Saccomanni D , Clementina Manera D and Piero A. Salvadori C + Author Affiliations - Author Affiliations A Nuclear Medicine Department, Prince of Wales Hospital, Barker Street, Randwick, NSW 2031, Australia.
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