[1] Oura, Y., Ebihara, M., Yoneda, S. and Nakamura, N. (2002) Chemical composition of the Kobe Meteorite; neutron-induced prompt gamma ray analysis study. Geochemical Journal, 36, 298-307.
[2] Randa, Z., Kucera, J. and Soukal, L. (2003) Elemental characterization of the new Czech meteorite ‘Moravka’ by neutron and photon activation analysis. Journal of Radioanalytical and Nuclear Chemistry, 257, 275-283. doi:10.1023/A:1024767309558
[3] Ebihara, M., Shinotsuka, K. and Kong, P. (1996) Chemical composition of Martian meteorites. 61st Annual Meteoritical Meeting, Germany.
[4] Larimer, J. W. (1971) Composition of the earth: Chondritic or achondritic? Geochimica et Cosmochimica Acta, 35, 769-786. doi:10.1016/0016-7037(71)90125-6
[5] Korotev, R. L. (2004) Lunar meteorites. Department of Earth and Planetary Sciences, Washington University, St. Louis.
[6] Ganzalez, M. A. (2003) Of meteors and meteorites. North Dakota Geological Survey, USA.
[7] Palme, H., Janssens, M.-J., Takahashi, H., Anders, E. and Hertogen, J. (1978) Meteoritic material at five large impact craters. Geochimica et Cosmochimica Acta, 42, 313-323. doi:10.1016/0016-7037(78)90184-9
[8] Nininger, H. H. (1992) An introduction to meteoritics. Dover Publications, Inc., New York.
[9] Meteorite phenomenon, the cratering process quantized. http://www.umich.edu/~gs265/meteor.htm