著書論文等- 中嶋 大輔 -
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件数:30件
[2011]
21.[] Oxygen isotope systematics of chondrules in Allende CV3 chondrite: High precision ion microprobe studies.[Geochimica et Cosmochimica Acta,75,(2011),7596-7611]Rudraswami N. G., Ushikubo T., Nakashima D., and Kita N. T.
10.1016/j.gca.2011.09.035
22.[] Ion microprobe analyses of oxygen three-isotope ratios of chondrules in the Sayh al Uhaymir 290 CH chondrite using a multiple-hole disk.[Meteoritics & Planetary Science,46,(2011),857-874]Nakashima D., Ushikubo T., Rudraswami N. G., Kita N. T., Valley J. W., and Nagao K.
10.1111/j.1945-5100.2011.01198.x
[2010]
23.[] Heavily fractionated noble gases in an acid residue from the Klein Glacier 98300 EH3 chondrite.[Geochimica et Cosmochimica Acta,74,(2010),5134-5149]Nakashima D., Ott U., El Goresy A., and Nakamura T.
10.1016/j.gca.2010.06.006
[2009]
24.[] CH3コンドライトSaU290のコンドリュールの希ガス同位体組成.[地球化学,43,(2009),133-142]中嶋大輔,長尾敬介
[2008]
25.[] Search for extinct 36Cl: Vigarano CAIs, the Pink Angel from Allende, and a Ningqiang chondrule.[Geochimica et Cosmochimica Acta,72,(2008),6141-6153]Nakashima D., Ott U., Hoppe P., and El Goresy A.
10.1016/j.gca.2008.10.001
[2007]
26.[] CAI中の短寿命放射性核種#U36#URClとその起源.[遊星人,16,(2007),146-150]中嶋大輔
[2006]
27.[] Cosmic-ray exposure age and heliocentric distance of the parent bodies of enstatite chondrites ALH85119 and MAC88136.[Meteoritics & Planetary Science,41,(2006),851-862]Nakashima D., Nakamura T., and Okazaki R.
28.[] Trapped noble gas components and exposure history of the enstatite chondrite ALH84206.[Geochemical Journal,40,(2006),543-555]Nakashima D. and Nakamura T.
[2003]
29.[] Formation history of CI-like Phyllosilicate-rich clasts in the Tsukuba meteorite inferred from mineralogy and noble gas signatures.[Earth and Planetary Science Letters,212,(2003),321-336]Nakashima D., Nakamura T., and Noguchi T.
10.1016/S0012-821x(03)00282-6
[2002]
30.[] Cosmic-ray exposure age and heliocentric distance of the parent body of H chondrites Yamato-75029 and Tsukuba.[Antarctic Meteorite Research,15,(2002),97-113]Nakashima D., Nakamura T., Sekiya M., and Takaoka N.
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