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We thank K. Nakamura-Messenger, T. Iwazumi, Y. Wakabayashi, A. Koyama, T. Mori, Y. Suzuki, A. Takeuchi, Y. Terada, H. Nagahara, and H. Yoshida for technical support; M. Sekiya, H. Miura, and M. Uesugi for discussion; and KEK and SPring-8 for experiments. This work was supported by the Japan Society for the Promotion of Science, the NASA Stardust Sample Analysis, and Cosmochemistry Programs. The Wisconsin Secondary Ion Mass Spectrometer Laboratory is partly supported by NSF
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We thank K. Nakamura-Messenger, T. Iwazumi, Y. Wakabayashi, A. Koyama, T. Mori, Y. Suzuki, A. Takeuchi, Y. Terada, H. Nagahara, and H. Yoshida for technical support; M. Sekiya, H. Miura, and M. Uesugi for discussion; and KEK and SPring-8 for experiments. This work was supported by the Japan Society for the Promotion of Science, the NASA Stardust Sample Analysis, and Cosmochemistry Programs. The Wisconsin Secondary Ion Mass Spectrometer Laboratory is partly supported by NSF.
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