p, He, and C to Fe cosmic-ray primary fluxes in diffusion models - Source and transport signatures on fluxes and ratios

A. Putze; D. Maurin; F. Donato

doi:doi:10.1051/0004-6361/201016064

Free access

Issue		A&A Volume 526, February 2011


Article Number		A101
Number of page(s)		19
Section		Astrophysical processes
DOI		http://dx.doi.org/10.1051/0004-6361/201016064
Published online		06 January 2011

Online material

Appendix A: Source slopes and relative elemental abundances

Table A.1

Most probable values and 68% CIs on the spectral index α and the relative source abundance q_Z/q_Si for the fit of the source spectrum parameters.

© ESO, 2011

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.

If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.