1984
DOI: 10.1016/b978-0-444-42273-6.50019-5
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Petrology of Megacrysts, Mafic and Ultramafic Xenoliths from the Pipe of Eglazines, Causses, France.

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1986
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Cited by 4 publications
(2 citation statements)
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“…Figure 1 contains the following sets of data: filled hexagon (HGLK); small filled circle (CGLK); open square (SLB) without garnet; filled and empty triangles (SLK; spinelbearing ultramafic in kimberlite; mainly lherzolites; with and without a titanate); cross (Fe-rich dunite xenoliths in Bultfontein kimberlite interpreted as aggregated olivine megacrysts (Dawson et al 1981)); m (mean of small range of olivine megacrysts in Bultfontein kimberlite (Dawson et al 1981)); d (inclusion in diamond (Hervig et al 1980b;Meyer & Boyd 1972;Prinz et al 1975;Meyer & Svisero 1975); only Cr 2 O 3 plotted for some inclusions); open diamond (GLM; also five olivines in garnet and spinel lherzolites, ); filled star (GHK, garnet harzburgite xenoliths in South African kimberlites (Berger & Vannier 1984)); w (garnet dunite xenoliths in Williams kimberlite (Hearn & McGee 1984)); open hexagon and small open circle (hot (HGLM) and cold (CGLM) garnet lherzolite xenoliths, respectively, greater and less than 1423 K in The Thumb minette (Ehrenberg 1982)); open star (spinel-garnet lherzolite xenolith in Eglazines basalt (Berger & Vannier 1984) and garnet lherzolite xenoliths in Salt Lake Crater basalt (Glassley & Piper 1978)). Because only eight SLK were analysed (Table 1), data were added for two spinel-garnet peridotites from the Frank Smith kimberlite (Exley et al 1982) and four spinel-garnet ultramafites from the Colorado-Wyoming kimberlites (Kirkley et al 1984).…”
Section: Olivinementioning
confidence: 99%
“…Figure 1 contains the following sets of data: filled hexagon (HGLK); small filled circle (CGLK); open square (SLB) without garnet; filled and empty triangles (SLK; spinelbearing ultramafic in kimberlite; mainly lherzolites; with and without a titanate); cross (Fe-rich dunite xenoliths in Bultfontein kimberlite interpreted as aggregated olivine megacrysts (Dawson et al 1981)); m (mean of small range of olivine megacrysts in Bultfontein kimberlite (Dawson et al 1981)); d (inclusion in diamond (Hervig et al 1980b;Meyer & Boyd 1972;Prinz et al 1975;Meyer & Svisero 1975); only Cr 2 O 3 plotted for some inclusions); open diamond (GLM; also five olivines in garnet and spinel lherzolites, ); filled star (GHK, garnet harzburgite xenoliths in South African kimberlites (Berger & Vannier 1984)); w (garnet dunite xenoliths in Williams kimberlite (Hearn & McGee 1984)); open hexagon and small open circle (hot (HGLM) and cold (CGLM) garnet lherzolite xenoliths, respectively, greater and less than 1423 K in The Thumb minette (Ehrenberg 1982)); open star (spinel-garnet lherzolite xenolith in Eglazines basalt (Berger & Vannier 1984) and garnet lherzolite xenoliths in Salt Lake Crater basalt (Glassley & Piper 1978)). Because only eight SLK were analysed (Table 1), data were added for two spinel-garnet peridotites from the Frank Smith kimberlite (Exley et al 1982) and four spinel-garnet ultramafites from the Colorado-Wyoming kimberlites (Kirkley et al 1984).…”
Section: Olivinementioning
confidence: 99%
“…The formation of the Velay migmatitic complex was established in the Upper Carboniferous, at the end of the collision episode that generated the Variscan Chain, which was built during a period from the Devonian to the Carboniferous (between 400 and 300 Ma). Beneath the Velay, the crust is strongly thinned, with a thickness of about 25 km (Mergoil and Boivin, 1993, and references therein) lying above a very heterogeneous lherzolitic mantle (Berger and Vannier, 1984). Tectonically, the Velay basement is affected by large northwest-southeast faults associated with northeast-southwest faults.…”
Section: The Velay Basementmentioning
confidence: 99%