COSMIC RAY ORIGIN IN OB ASSOCIATIONS AND PREFERENTIAL ACCELERATION OF REFRACTORY ELEMENTS: EVIDENCE FROM ABUNDANCES OF ELEMENTS Fe-26 THROUGH Se-34

Record Type
Journal Articles
Full Title
COSMIC RAY ORIGIN IN OB ASSOCIATIONS AND PREFERENTIAL ACCELERATION OF REFRACTORY ELEMENTS: EVIDENCE FROM ABUNDANCES OF ELEMENTS Fe-26 THROUGH Se-34
Author(s)
Rauch B, Link J, Lodders K, Israel M, Barbier L, Binns W, Christian E, Cummings J, de Nolfo G, Geier S, Mewaldt R, Mitchell J, Schindler S, Scott L, Stone E, Streitmatter R, Waddington C, Wiedenbeck M
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2009 Jun 1
DOI
10.1088/0004-637X/697/2/2083
ISSN
0004-637X
Volume
697
Issue
2
Page Count
6
First Page
2083
Last Page
2088
Keyword(s)
Astronomy & Astrophysics, cosmic rays, Galaxy: abundances, ISM: abundances, stars: winds, outflows, ISOTOPIC COMPOSITION, SUPERBUBBLE ORIGIN, SUPERNOVA-REMNANTS, CROSS-SECTIONS, MASSIVE STARS, NUCLEI, NEON, CHARGE, NUCLEOSYNTHESIS, HYDROGEN
Citation
Rauch B, Link J, Lodders K, Israel M, Barbier L, Binns W, Christian E, Cummings J, de Nolfo G, Geier S, et al. COSMIC RAY ORIGIN IN OB ASSOCIATIONS AND PREFERENTIAL ACCELERATION OF REFRACTORY ELEMENTS: EVIDENCE FROM ABUNDANCES OF ELEMENTS Fe-26 THROUGH Se-34. ASTROPHYS J. 2009;697 (2):2083-2088.
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