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Cosmic-Ray Neon, Wolf-Rayet Stars, and the Superbubble Origin of Galactic Cosmic Rays

Binns, W. R. and Wiedenbeck, M. E. and Arnould, M. and Cummings, A. C. and George, J. S. and Goriely, S. and Israel, M. H. and Leske, R. A. and Mewaldt, R. A. and Meynet, G. and Scott, L. M. and Stone, E. C. and von Rosenvinge, T. T. (2005) Cosmic-Ray Neon, Wolf-Rayet Stars, and the Superbubble Origin of Galactic Cosmic Rays. Astrophysical Journal, 634 (1). pp. 351-364. ISSN 0004-637X. doi:10.1086/496959.

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We report the abundances of neon isotopes in the Galactic cosmic rays (GCRs) using data from the Cosmic Ray Isotope Spectrometer (CRIS) aboard the Advanced Composition Explorer (ACE). These abundances have been measured for seven energy intervals over the energy range of 84 ≤ E/M ≤ 273 MeV nucleon^(-1). We have derived the ^(22)Ne/^(20)Ne ratio at the cosmic-ray source using the measured ^(21)Ne, ^(19)F, and ^(17)O abundances as "tracers" of secondary production of the neon isotopes. Using this approach, the ^(22)Ne/^(20)Ne abundance ratio that we obtain for the cosmic-ray source is 0.387 ± 0.007(statistical) ± 0.022(systematic). This corresponds to an enhancement by a factor of 5.3 ± 0.3 over the ^(22)Ne/^(20)Ne ratio in the solar wind. This cosmic-ray source ^(22)Ne/^(20)Ne ratio is also significantly larger than that found in anomalous cosmic rays, solar energetic particles, most meteoritic samples of matter, and interplanetary dust particles. We compare our ACE CRIS data for neon and refractory isotope ratios, and data from other experiments, with recent results from two-component Wolf-Rayet (W-R) models. The three largest deviations of GCR isotope ratios from solar system ratios predicted by these models, ^(12)C/^(16)O, ^(22)Ne/^(20)Ne, and ^(58)Fe/^(56)Fe, are indeed present in the GCRs. In fact, all of the isotope ratios that we have measured are consistent with a GCR source consisting of about 80% material with solar system composition and about 20% W-R material. Since W-R stars are evolutionary products of OB stars, and most OB stars exist in OB associations that form superbubbles, the good agreement of these data with W-R models suggests that superbubbles are the likely source of at least a substantial fraction of GCRs.

Item Type:Article
Related URLs:
URLURL TypeDescription Paper
Binns, W. R.0000-0001-6110-3407
Wiedenbeck, M. E.0000-0002-2825-3128
Cummings, A. C.0000-0002-3840-7696
Israel, M. H.0000-0002-8104-208X
Leske, R. A.0000-0002-0156-2414
Mewaldt, R. A.0000-0003-2178-9111
Stone, E. C.0000-0002-2010-5462
Additional Information:© 2005 American Astronomical Society. Received 2005 June 30; accepted 2005 August 4. We wish to thank Katharina Lodders of Washington University for helpful discussions on the fraction of elements tied up in grains in the solar system interplanetary medium. We also wish to thank Sachiko Amari, Charles Hohenberg, and Ernst Zinner for helpful discussions on neon in meteorites. This research was supported by the National Aeronautics and Space Administration at the California Institute of Technology (under grants NAG5-6912 and NAG5-12929), Washington University, the Jet Propulsion Laboratory, and the Goddard Space Flight Center.
Group:Space Radiation Laboratory
Funding AgencyGrant Number
Washington UniversityUNSPECIFIED
Goddard Space Flight CenterUNSPECIFIED
Subject Keywords:cosmic rays; Galaxy: abundances; Galaxy: stellar content; stars: Wolf-Rayet
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Other Numbering System NameOther Numbering System ID
Space Radiation Laboratory2005-05
Issue or Number:1
Record Number:CaltechAUTHORS:20140827-093644016
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Official Citation:Cosmic-Ray Neon, Wolf-Rayet Stars, and the Superbubble Origin of Galactic Cosmic Rays W. R. Binns et al. 2005 ApJ 634 351
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:48974
Deposited By: Ruth Sustaita
Deposited On:27 Aug 2014 17:55
Last Modified:10 Nov 2021 18:38

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