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LINE EMISSION FROM THE INNER GALAXY<br />
[23] Predicted power in ultra high energy cosmic rays<br />
from active galaxies, Laurentiu I. Caramete, Oana<br />
Tascau, <strong>Peter</strong> L. Biermann and Todor Stanev, submitted<br />
Astron. & Astroph. (2011); arXiv:1106.5109<br />
[24] Cosmic rays I. The cosmic ray spectrum between 104 GeV and 3 109 GeV, <strong>Peter</strong> L. Biermann, Astron. &<br />
Astroph. 271, 649 (1993), astro-ph/9301008<br />
40<br />
[25] Cosmic rays II. Evidence for a magnetic rotator<br />
Wolf-Rayet star origin, <strong>Peter</strong> L. Biermann, & Joseph<br />
P. Cassinelli, Astron. & Astroph. 277, 691 (1993);<br />
astro-ph/9305003<br />
[26] Cosmic Rays III. The cosmic ray spectrum between<br />
1 GeV and 104 GeV and the radio emission from supernova<br />
remnants, <strong>Peter</strong> L. Biermann, & Richard G.
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