1. Alekseeva, K.N., The physical properties of stony meteorites and their interpretation in the context of the hypothesis of meteorite origin, Meteoritika, 1958, no. 6, pp. 67–77.
2. Anders, E., How well do we know “Cosmic” abundances? Geochim. Cosmochim. Acta, 1971, vol. 35, pp. 516–522.
3. Barsukova, L.D., Kharitonova, V.Ya., and Bannykh, L.N., Chemical composition of Tsarev meteorite, Meteoritika, 1982, no. 41, pp. 41–43.
4. Bischoff, A., Dyl, K.A., Horstmann, M., Ziegler, K., Wimmer, K., and Young, E.D., Reclassification of Villalbeto de la Peña—occurrence of a winonaite-related fragment in a hydrothermally metamorphosed polymict L-chondritic breccia, Meteorit. Planet. Sci., 2013, vol. 48, pp. 628–640.
5. Bischoff, A., Jersek, M., Grau, T., Mirtic, B., Ott, U., Kucera, J., Horstmann, M., Laubenstein, M., Herrmann, S., Randa, Z., Weber, M., and Heusser, G., Jesenice—a new meteorite fall from Slovenia, Meteorit. Planet. Sci., 2011, vol. 46, pp. 793–804.