A New Determination of the 12C/13C Abundance Ratio in the Solar Photosphere.

1966 ◽  
Vol 71 ◽  
pp. 383
Author(s):  
L. Delbouille ◽  
Luise Herzberg ◽  
G. Roland
1967 ◽  
Vol 147 ◽  
pp. 697 ◽  
Author(s):  
Luise Herzberg ◽  
L. Delbouille ◽  
G. Roland

2000 ◽  
Vol 198 ◽  
pp. 415-424
Author(s):  
Katia Cunha

Although the behavior of boron versus metallicity has been probed in a fairly large sample of halo dwarfs with HST, it is only very recently that boron abundances have been derived systematically in solar metallicity dwarfs. This effort began with a re-analysis of the solar spectrum with modern atomic data and model atmospheres so that the Sun could be adopted as a standard for the calibration of a line list in the region of the B I transition at 2497 Â. The solar analysis indicates that boron is not depleted in the solar photosphere. From a subsequent study of a sample of 14 field F/G-dwarfs with roughly solar metallicities, it is found that the behavior of boron versus [Fe/H] follows the linear trend that is observed for the halo stars. The average B/Be obtained for solar metallicity stars is 27±5 compared to the solar ratio of 23. The determination of boron abundances in the young B-type and G-type stars of the Orion association reveals a behavior of boron and oxygen in Orion that is opposite of the positive correlation which is observed for the field stars: the boron and oxygen abundances are anticorrelated.


2001 ◽  
Vol 65 (24) ◽  
pp. 4589-4596 ◽  
Author(s):  
James M. Weygand ◽  
Fred M. Ipavich ◽  
Peter Wurz ◽  
John A. Paquette ◽  
Peter Bochsler

2015 ◽  
Vol 799 (2) ◽  
pp. 150 ◽  
Author(s):  
Christopher S. Moore ◽  
Han Uitenbroek ◽  
Matthias Rempel ◽  
Serena Criscuoli ◽  
Mark P. Rast

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