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  • 1
    ISSN: 1520-4995
    Source: ACS Legacy Archives
    Topics: Biology , Chemistry and Pharmacology
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 287 (1980), S. 787-790 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The Tieschitz unequilibrated H-group chondrite accreted at (800±100) °C during rapid cooling 11. From their mineral chemistry, nine other H-group chondrites, exhibiting greater degrees of equilibration, also formed hot. Degree of equilibration is equated with slowness of ...
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  • 3
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 280 (1979), S. 116-119 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The Tieschitz, H3, chondritic meteorite apparently formed as part of a parent-body by the accretion of both molten and solid materials with a mean temperature of 800±100 °C, followed by slow cooling to lower temperatures. Our data argue against the currently accepted model of ...
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  • 4
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 263 (1976), S. 302-303 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Our British Museum specimen (BM 67215) mates with that shown in Fig. 3 of ref. 1. Most of our general microscopic observations are in agreement with those of Buchwald2. We found that phosphide is absent, daubreelite is present as rare particles, and troilite is present in varying degrees of shock ...
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  • 5
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 301 (1983), S. 322-324 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] Solid-state precipitation processes recognized so far in meteoritic Fe,Ni metal mainly involve the growth of a new phase by means of a 'volume' diffusion flux perpendicular to the growing interface. The best known example is the development of the Widmansttten structure in the octahedrite classes ...
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  • 6
    ISSN: 1432-1017
    Keywords: Dihydrofolate reductase ; trimethoprim ; NMR (15N, 1H) ; hydrogen bonding ; protonation
    Source: Springer Online Journal Archives 1860-2000
    Topics: Biology , Physics
    Notes: Abstract The binding of trimethoprim and [1,3,2-amino-15N3]-trimethoprim to Lactobacillus casei dihydrofolate reductase has been studied by 15N and 1H NMR spectroscopy. 15N NMR spectra of the bound drug were obtained by using polarisation transfer pulse sequences. The 15N chemical shifts and 1H-15N spin-coupling constants show unambiguously that the drug is protonated on N1 when bound to the enzyme. The N1-proton resonance in the complex has been assigned using the 15N-enriched molecule. The temperature-dependence of the linewidth of this resonance has been used to estimate the rate of exchange of this proton with the solvent: 160±10s-1 at 313 K, with an activation energy of 75 (±9) kJ·mole-1. This is considerably faster than the dissociation rate of the drug from this complex, demonstrating that there are local fluctuations in the structure of the complex.
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  • 7
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    In:  Geological Society Special Publication 256: 325-343.
    Publication Date: 2007-10-08
    Description: During the last 35 years, the number of meteorites available for study has increased by an order of magnitude (from around 2000 to nearly 30 000). The largest contribution has come from meteorites recovered from the Antarctic ice (more than 20 000); however, since the late 1980s a significant number (more than 8000-9000) have come from so called hot' deserts. The most notable arid areas of the world for meteorite recoveries are the wider Sahara (Algeria, Libya, Niger and other unspecified localities in NW Africa), Roosevelt County in New Mexico, USA, the Nullarbor Region of Australia, and, more recently, the deserts of the Arabian Peninsula in Saudi Arabia and Oman. Other areas in which meteorites have been found in numbers include the Namibian Desert in SW Africa and the Atacama Desert in Chile. This wealth of material has greatly extended our knowledge of early solar system materials by providing occasional samples of meteorites hitherto unknown to science, and allowing the construction of new groups of related meteorites. In addition, these accumulated collections have also allowed estimates to be made of the flux of meteorites to Earth with time, studies of their mass/type distribution on Earth and palaeoclimatic studies of the areas from which meteorites have been recovered. This paper documents the history of meteorite recovery from the hot' deserts of the world, and notes the effects that this abundance of material has had on the science of meteoritics. ... This 250-word extract was created in the absence of an abstract.
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  • 8
    facet.materialart.
    Unknown
    In:  Geological Society Special Publication 256: 305-323.
    Publication Date: 2007-10-08
    Description: The first meteorites recovered from Western Australia were a number of irons, the earliest of which was found in 1884 east of the settlement of York. These were named the Youndegin' meteorites after a police outpost. Some of the larger specimens were taken to London to be sold as scrap metal, but were recognized as meteorites and eventually acquired by museums. The main mass of Youndegin (2626 kg) was recovered in 1954 and is retained in the collection of the Western Australian Museum. Despite a sparse population and relatively recent settlement by Europeans (1829), a number of factors have contributed to the excellent record of meteorite recovery in Western Australia. Primarily, large regions of arid land have allowed meteorites to be preserved for millennia, and these are generally easily distinguished from the country rocks. A less obvious, but significant, factor is that, in antiquity, Australian Aborigines do not appear to have utilized meteorites extensively. Finally, systematic collecting from the Nullarbor Region, has contributed to the large numbers of recoveries since 1969. The Father' of the State's meteorite collection was the chemist and mineralogist Edward Sydney Simpson (1875-1939) who, from 1897 to 1939, recorded and analysed many of the meteorites that formed the foundation of the collection. The first Catalogue of Western Australian Meteorites was published by McCall & de Laeter in 1965 (Western Australian Museum, Special Publications, 3). Forty-eight meteorites were listed, 29 of which were irons (some of which have since been paired). Interest in meteorites increased in the 1960s, so that when the second supplement to the catalogue was published in 1972, 92 meteorites were listed with stones accounting for most of the additional recoveries. Today, the collection contains thousands of specimens of 248 distinct meteorites from Western Australia (218 stones, 26 irons and four stony-irons), and around 500 samples of potentially new meteorites (mostly chondrites from the Nullarbor) that remain to be examined. There are also specimens of 160 meteorites from other parts of Australia and the rest of the world. While numerically the collection is small compared to other major collections in the world, it contains a high percentage of main masses from Western Australia (around 85%), including many rarities, and has an aggregate weight in excess of 20 tonnes. The small proportion of falls to finds (4: 244) reflects the sparse population of the State. This may change significantly when a network of all-sky fireball cameras is established in the Nullarbor Region. ... This 250-word extract was created in the absence of an abstract.
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  • 9
    Publication Date: 1968-02-01
    Print ISSN: 0021-8979
    Electronic ISSN: 1089-7550
    Topics: Physics
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  • 10
    Publication Date: 1963-04-01
    Print ISSN: 0021-9606
    Electronic ISSN: 1089-7690
    Topics: Chemistry and Pharmacology , Physics
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