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NSR database version of April 27, 2024.

Search: Author = E.C.Stone

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2009RA07      Astrophys.J. 697, 2083 (2009)

B.F.Rauch, J.T.Link, K.Lodders, M.H.Israel, L.M.Barbier, W.R.Binns, E.R.Christian, J.R.Cummings, G.A.de Nolfo, S.Geier, R.A.Mewaldt, J.W.Mitchell, S.M.Schindler, L.M.Scott, E.C.Stone, R.E.Streitmatter, C.J.Waddington, M.E.Wiedenbeck

Cosmic ray origin in OB associations and preferential acceleration of refractory elements: evidence from abundances of elements ₂₆Fe through ₃₄Se

doi: 10.1088/0004-637X/697/2/2083
Citations: PlumX Metrics

2005IS10      Nucl.Phys. A758, 201c (2005)

M.H.Israel, W.R.Binns, A.C.Cummings, R.A.Leske, R.A.Mewaldt, E.C.Stone, T.T.von Rosenvinge, M.E.Wiedenbeck

Isotopic Composition of Cosmic Rays: Results from the Cosmic Ray Isotope Spectrometer on the ACE Spacecraft

doi: 10.1016/j.nuclphysa.2005.05.038
Citations: PlumX Metrics

1990CU07      Phys.Rev. C 42, 2508 (1990)

J.R.Cummings, W.R.Binns, T.L.Garrard, M.H.Israel, J.Klarmann, E.C.Stone, C.J.Waddington

Determination of the cross sections for the production of fragments from relativistic nucleus-nucleus interactions. I. Measurements

NUCLEAR REACTIONS H(¹⁹⁷Au, x), H(¹⁶⁵Ho, x), H(¹³⁹La, x), ¹H(¹⁶⁵Ho, x), ¹H(¹³⁹La, x), ¹²C(¹⁹⁷Au, x), ¹²C(⁵⁶Fe, x), ¹²C(¹⁶⁵Ho, x), ¹²C(¹³⁹La, x), ²⁷Al(¹⁹⁷Au, x), ²⁷Al(⁵⁶Fe, x), ²⁷Al(¹⁶⁵Ho, x), ²⁷Al(¹³⁹La, x), Cu(¹⁹⁷Au, x), Cu(⁵⁶Fe, x), Cu(¹⁶⁵Ho, x), Cu(¹³⁹La, x), ²⁰⁸Pb(⁵⁶Fe, x), E=71.5-180.2 GeV; measured products; deduced σ, σ(E). Data were imported from EXFOR entry C1874.

doi: 10.1103/PhysRevC.42.2508
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1874.