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.
Journals Menu
Follow SCIRP
Contact us
+1 323-425-8868
customer@scirp.org
WhatsApp +86 18163351462(WhatsApp)
Click here to send a message to me 1655362766
Paper Publishing WeChat

Copyright © 2024 by authors and Scientific Research Publishing Inc.

Creative Commons License

This work and the related PDF file are licensed under a Creative Commons Attribution 4.0 International License.