International Journal of Astronomy and Astrophysics

Vol.2 No.1(2012), Paper ID 18181, 2 pages

DOI:10.4236/ijaa.2012.21006

 

Why Do the Main Sequence Stars Have Similar Chemical Composition?

 

Stanislaw Halas, Tomasz Durakiewicz

 

Institute of Physics, Maria Curie-Sklodowska University, Lublin, Poland
Los Alamos National Laboratory, MPA-CMMS Group, Los Alamos, USA

 

Copyright © 2012 Stanislaw Halas, Tomasz Durakiewicz et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

 

How to Cite this Article


S. Halas and T. Durakiewicz, "Why Do the Main Sequence Stars Have Similar Chemical Composition?," International Journal of Astronomy and Astrophysics, Vol. 2 No. 1, 2012, pp. 37-38. doi: 10.4236/ijaa.2012.21006.

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