| | Book | 352 Figures Springer-Verlag, Berlin Heidelberg New York London Paris Tokyo Prof. Dr. JOSEPH V. SMITH...that a completely new version of Feldspar Minerals was needed because of the important new results on the...I would turn the original Volumes 1 and 2 into a new Volume 1, and all three of us would share the preparation...inserted. It was impractical to continue adding all the new data to the complex figures, especially of Chapter...and proof-reading. It was necessary to switch to a new word processor in December 1986. Because we did not | | | Book (edition) | photograph their specimens for this book. Front co,·er photos: Turquoise, polished. 55 mm, ZhiJandy...Rhodocbrosite, polished, 50 mm, Capillitas, Argentina, H Back cO\·erphoto: Wolframite. 45 mm. Yaogangxian, China,...The current progress in mineralog), with countless new data in books and scientific as well as amateur journals...submitted to, and accepted by, the Commission on New Minerals and Mineral Names (CNMMN) of the International...pure freibergite is very rare. The decision that a new mineral species is established when one of the cations | | | Book | responsibility for authors’ errors and omissions. SOUTH AFRICA SEVENTH INTERNATIONAL KIMBERLITE CONFERENCE...Survey of South Africa) SouthemEra Resources Ltd SOCIETY SPONSORS Geological Society of South Africa (GSSA)...Phanerozoic subduction regime in eastern New South Wales, Australia. Mantle Dynamics beneath Mongolia: Implications...gamet-pyroxenite xenoliths from Siberian kimberlites, a new N.P., Orihashi, Y. insight into lithospheric mantle...Lithospheric Mantle anisotropy of the Kaapvaal craton (South Africa) from lattice preferred orientation analysis | | | Book | heavyelement-enriched matter to the interstellar gas from which new stars are formed. The mass fraction of our solar...accompanied by significant mass loss, and they evolve to white dwarfs of carbon– oxygen (or, less commonly, oxygen...can leave in its wake compact stellar remnants: white dwarfs, neutron stars, and black holes. Indeed,...hydrogen thermonuclear runaways in accreted shells on white dwarfs (Gehrz et al., 1998)), X-ray bursts (hydrogen/helium...accretion onto carbon – oxygen white dwarfs will permit growth of the CO core to the Chandrasekhar limit |
|