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  • Articles  (228)
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  • 1
    Electronic Resource
    Electronic Resource
    s.l. : American Chemical Society
    Accounts of chemical research 8 (1975), S. 217-224 
    ISSN: 1520-4898
    Source: ACS Legacy Archives
    Topics: Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 249 (1974), S. 333-334 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The Allende samples can be grouped in various ways using chemical, mineralogical and textural parameters. Our results distinguish four distinct groups, as follows: group I, melilite-rich chondrules; group II, CaAl-rich aggregates with fractionated chondrite-normalised REE abundance patterns; ...
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  • 3
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 183 (1959), S. 254-255 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] One may reasonably ask which are these "more acid sedimentary rocks" to which Prof. Urey refers. I do not know any publication in which analyses of tektites are directly compared with those of sedimentary rocks. The most comprehensive compilation of tek-tite analyses is that of Barnes2. In ...
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 186 (1960), S. 230-231 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] I would suggest an alternative hypothesis, that the structure of chondritic meteorites is the result of reaction and recrystallization of pre-existing material essentially in the solid state, and that many, if not all, chondritic meteorites, instead of being fragments of a disrupted planet or ...
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  • 5
    Electronic Resource
    Electronic Resource
    Springer
    Space science reviews 1 (1963), S. 621-646 
    ISSN: 1572-9672
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract The carbonaceous chondrites are a group of stony meteorites characterized by the presence of an appreciable amount of carbonaceous material other than free carbon (diamond and graphite). They have been divided into three subgroups known respectively as Type I, Type II, and Type III. Analyses of Type I meteorites show about 3–5% of carbon and 20% of combined water; they consist largely of hydrated magnesium-iron silicate, magnetite, and magnesium sulfate, contain no chondrules, and have a density about 2.2. Analyses of Type II meteorites show about 2–3% of carbon and 10–15% of combined water; they consist of a groundmass of hydrated magnesium-iron silicate enclosing chondrules of olivine and pyroxene which are almost iron-free, and have a density of 2.6–2.9. Analyses of Type III meteorites show about 0.5–2% of carbon and 2% combined water; they consist largely of olivine (often variable in composition, but averaging 30–40 mole per cent Fe2SiO4), with accessory pigeonite and sulfide minerals, and have a density about 3.4. The carbonaceous material and combined water in these meteorites are clearly of extraterrestrial origin, but their significance is not well understood. A biological origin has been claimed for some of the organic compounds on the basis of their composition, but this claim is the subject of considerable dispute. Microscopic objects with regular outline (“organized elements”) have been recognized in some of these meteorites; some investigators have claimed these to be extraterrestrial fossils, others have ascribed them to terrestrial contamination or considered them to be crystals or crystal aggregates of non-biological origin.
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  • 6
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 211 (1966), S. 616-618 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Of the two major groups of chondritic meteorites, the olivine-bronzite and olivine-hypersthene chondrites, the average composition of the bronzite chondrites2 is close to Birch's initial requirement. Table 1 shows an FeO content of 9-7 per cent, equivalent to 12*6 per cent FeO in the silicate ...
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  • 7
    ISSN: 1432-1203
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Abstract The correlation between mutations in the Werner’s syndrome (WRN) gene and the haplotypes of surrounding markers was studied in Japanese patients. We have elucidated the genomic structure of WRN helicase, and found five additional mutations, designated mutations 6–10. Mutations 4 and 6 were found to be the two major mutations in this population; these mutations comprised 50.8% and 17.5%, respectively, of the total in a sample of 126 apparently unrelated chromosomes. Almost all the patients homozygous for mutation 4 shared a haplotype around the WRN gene, consistent with the view that they are derived from a single ancestor. This important advantage demonstrated in the identification of the WRN gene suggests that the Japanese present a unique population for the cloning of other disease genes. The conserved haplotype was observed across 19 loci, extending a distance estimated to be more than 1.4 Mbp around the WRN gene. This haplotype is rare among random Japanese individuals. Unexpectedly, all the nine patients homozygous for mutation 6 shared a haplotype that was identical to this haplotype at 18 of these 19 markers. These results suggest that mutations 4 and 6 arose independently in almost identical rare haplotypes. The remaining mutations (1, 5, 7, 8, 9, and 10) occurred rarely, and were each associated with different haplotypes.
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  • 8
    ISSN: 1432-1203
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Medicine
    Notes: Abstract The profile of helicase gene mutations was studied in 89 Japanese Werner’s syndrome (WRN) patients by examining the previously described mutations 1– 4 as well as a new mutation found during this study, designated mutation 5. Of 178 chromosomes (89 patients), 89 chromosomes (50%) had mutation 4, 11 (6.2%) chromosomes had mutation 1, and two chromosomes (1.1%) contained mutation 5. Mutations 2 and 3 were not observed in this patient population. The remaining 76 (42.7%) chromosomes had none of these mutations. A significant fraction of all patients (22 total patients, 24.7%) appear to be compound heterozygotes, including those carrying mutations of both types 1 and 4. The genotype analysis of the markers surrounding the WRN helicase gene strongly suggests that most of the chromosomes carrying either mutation 1 or 4 were derived from two single founders.
    Type of Medium: Electronic Resource
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  • 9
    Electronic Resource
    Electronic Resource
    Springer
    Contributions to mineralogy and petrology 19 (1968), S. 316-327 
    ISSN: 1432-0967
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract Eclogitic xenoliths consisting of tschermakitic augite and pyrope garnet, together with variable amounts of kaersutitic hornblende, are common in a volcanic breccia of Lower Oligocene age at Kakanui, New Zealand. The breccia also contains xenocrysts of these minerals, and xenoliths of peridotite. Modal analyses are given of a number of the eclogitic xenoliths, and chemical analyses of two of them and their component minerals. They are compared with similar xenoliths from Hoggar (Algeria), Salt Lake Crater (Hawaii), and Delegate (Australia), with eclogite xenoliths from kimberlites, and with garnet peridotites. These three types of igneous eclogites can be characterized by the nature of their clinopyroxene: tschermakitic in the xenoliths from basaltic rocks, jadeitic in the xenoliths from kimberlites, and chrome diopside in the garnet peridotites. The eclogitic xenoliths in basaltic rocks probably crystallized in the mantle at depths of about 60 km, but their rarity in contrast to the numerous occurrences of peridotite xenoliths poses some significant problems.
    Type of Medium: Electronic Resource
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  • 10
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