Extraterrestrial Helium Trapped in Fullerenes in the Sudbury Impact Structure
暂无分享,去创建一个
[1] Martin Saunders,et al. Stable Compounds of Helium and Neon: He@C60 and Ne@C60 , 1993, Science.
[2] E. Anders,et al. Interstellar graphite in meteorites , 1990, Nature.
[3] K. Farley,et al. Rare gases in Samoan xenoliths , 1992 .
[4] H. Jiménez-Vázquez,et al. Hot-atom incorporation of tritium atoms into fullerenes , 1994 .
[5] D. Brownlee,et al. Helium and neon isotopes in deep Pacific Ocean sediments , 1990 .
[6] H. Kroto,et al. Space, Stars, C60, and Soot , 1988, Science.
[7] C. Chyba,et al. Cometary delivery of organic molecules to the early Earth. , 1990, Science.
[8] J. Bada,et al. Fullerenes in the 1.85-billion-year-old Sudbury impact structure. , 1994, Science.
[9] J. Morgan,et al. Extinct Superheavy Element in the Allende Meteorite , 1975, Science.
[10] D. Bohme,et al. Ab initio MO calculation on the energy barrier for the penetration of a benzene ring by a helium atom. Model studies for the formation of endohedral He@C60+ complexes by high-energy bimolecular reactions , 1992 .
[11] J. Bada,et al. Fullerenes in Allende meteorite , 1994, Nature.
[12] Martin Saunders,et al. Noble Gas Atoms Inside Fullerenes , 1996, Science.
[13] R. Wieler,et al. He, Ne, and Ar from the solar wind and solar energetic particles in lunar ilmenites and pyroxenes , 1993 .
[14] K. Farley. Cenozoic variations in the flux of interplanetary dust recorded by3He in a deep-sea sediment , 1995, Nature.
[15] U. Ott,et al. Noble-gas-rich separates from the Allende meteorite , 1981 .
[16] A. Tielens,et al. Interstellar polycyclic aromatic hydrocarbons: the infrared emission bands, the excitation/emission mechanism, and the astrophysical implications. , 1989, The Astrophysical journal. Supplement series.
[17] D. Bohme. PAH and Fullerene Ions and Ion/Molecule Reactions in Interstellar and Circumstellar Chemistry , 1992 .
[18] B. Foing,et al. Detection of two interstellar absorption bands coincident with spectral features of C60+ , 1994, Nature.
[19] W. Krätschmer,et al. Solid C60: a new form of carbon , 1990, Nature.
[20] M. Kurz,et al. Constraints on evolution of Earth's mantle from rare gas systematics , 1983, Nature.
[21] D. Bohme,et al. Experimental results for ion-molecule reactions of fullerenes: implications for interstellar and circumstellar chemistry , 1993 .
[22] Carl Sagan,et al. Endogenous production, exogenous delivery and impact-shock synthesis of organic molecules: an inventory for the origins of life , 1992, Nature.
[23] A. Nier,et al. Extraction of helium from individual interplanetary dust particles by step-heating , 1992 .
[24] N. Ohmi,et al. Direction finding of ELF hiss emissions in a detached plasma region of the magnetosphere , 1986 .
[25] C. Pillinger,et al. Interstellar Carbon in Meteorites , 1983, Science.
[26] Harold W. Kroto,et al. A postbuckminsterfullerene view of carbon in the galaxy , 1992 .
[27] A. Witt,et al. The Interstellar Carbon Budget and the Role of Carbon in Dust and Large Molecules , 1995, Science.
[28] H. Craig,et al. Geomorphology and In-Situ Cosmogenic Isotopes , 1994 .
[29] D. Lal. An important source of4He (and3He) in diamonds , 1989 .
[30] John F. Kerridge,et al. Meteorites and the early solar system , 1988 .
[31] T. Robl,et al. Comparison of the HF−HCl and HF−BF3 maceration techniques and the chemistry of resultant organic concentrates , 1993 .