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Books on the topic 'Carbene precursor'

Author: Grafiati
Published: 4 June 2021
Last updated: 8 February 2022

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1

Brauer, Samuel. Advanced structural fibers from precursors: Carbon, silicon carbide. Norwalk, CT: Business Communications Co., 1997.

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2

Naskar, Amit K., and Wesley P. Hoffman, eds. Polymer Precursor-Derived Carbon. Washington, DC: American Chemical Society, 2014. http://dx.doi.org/10.1021/bk-2014-1173.

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3

White, Robin J., ed. Porous Carbon Materials from Sustainable Precursors. Cambridge: Royal Society of Chemistry, 2015. http://dx.doi.org/10.1039/9781782622277.

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4

Gardner, LuAnn. Procedures for the preparation of emission inventories for carbon monoxide and precursors of ozone. Research Triangle Park, NC: Office of Air Quality Planning and Standards, Office of Air and Reduction, U.S. Environmental Protection Agency, 1992.

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5

Gardner, LuAnne. Procedures for the preparation of emission inventories for carbon monoxide and precursors of ozone. Research Triangle Park, NC: Office of Air Quality Planning and Standards, Office of Air and Reduction, U.S. Environmental Protection Agency, 1992.

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6

Gardner, LuAnn. Procedures for the preparation of emission inventories for carbon monoxide and precursors of ozone. Research Triangle Park, NC: Office of Air Quality Planning and Standards, Office of Air and Reduction, U.S. Environmental Protection Agency, 1992.

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7

Gardner, LuAnn. Procedures for the preparation of emission inventories for carbon monoxide and precursors of ozone. Research Triangle Park, NC: Office of Air Quality Planning and Standards, Office of Air and Reduction, U.S. Environmental Protection Agency, 1992.

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8

Speiran, Gary K. Dissolved organic carbon and disinfection by-product precursors in waters of the Chickahominy River basin, Virginia, and implications for public supply. Richmond, Va: U.S. Dept. of the Interior, U.S. Geological Survey, 2000.

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9

Speiran, Gary K. Dissolved organic carbon and disinfection by-product precursors in waters of the Chickahominy River basin, Virginia, and implications for public supply. Richmond, Va: U.S. Dept. of the Interior, U.S. Geological Survey, 2000.

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10

Polymer Precursor-Derived Carbon. American Chemical Society, 2015.

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11

Matzinos, Panagiotis D. Coal-tar pitch as the matrix carbon precursor in carbon-carbon composites. 1995.

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12

Zhao, Li, Rafael Luque, Rezan Demir-Cakan, Robin J. White, and Noriko Yoshizawa. Porous Carbon Materials from Sustainable Precursors. Royal Society of Chemistry, The, 2015.

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13

Delhaes, Pierre. Graphite and Precursors (World of Carbon). CRC, 2000.

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14

Awwa Research Foundation (Corporate Author), Douglas M. Owen (Editor), and R. Scott Summers (Editor), eds. Removal of Dbp Precursor by Granular Activated Carbon Absorption. Amer Water Works Assn, 1998.

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15

United States. National Aeronautics and Space Administration., ed. Carbon-rich ceramic composites from ethynyl aromatic precursors. [Washington, DC: National Aeronautics and Space Administration, 1986.

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16

United States. National Aeronautics and Space Administration., ed. Carbon-rich ceramic composites from ethynyl aromatic precursors. [Washington, DC: National Aeronautics and Space Administration, 1986.

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17

Carbon-rich ceramic composites from ethynyl aromatic precursors. [Washington, DC: National Aeronautics and Space Administration, 1986.

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18

United States. National Aeronautics and Space Administration., ed. Carbon-rich ceramic composites from ethynyl aromatic precursors. [Washington, DC: National Aeronautics and Space Administration, 1986.

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19

Myram, Sarah Frances. Modification of coal-tar pitch for use as a precursor for matrix carbon in carbon-carbon composites. 1998.

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20

Removal of DBP precursors by GAC absorption. Denver, CO: AWWA Research Foundation and American Water Works, 1998.

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21

Arlander, Dixon William. Measurements of organic acids and their precursors in the remote marine troposphere. 1988.

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22

Hernndez Montoya, Virginia, ed. Lignocellulosic Precursors Used in the Synthesis of Activated Carbon - Characterization Techniques and Applications in the Wastewater Treatment. InTech, 2012. http://dx.doi.org/10.5772/3346.

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23

G, Penn B., and George C. Marshall Space Flight Center., eds. Preparation of silicon carbide-silicon nitride fibers by the pyrolysis of polycarbosilazane precursors: (Center director's Discretionary Fund final report). [Marshall Space Flight Center, Ala.]: National Aeronautics and Space Administration, George C. Marshall Space Flight Center, 1985.

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24

Preparation of silicon carbide-silicon nitride fibers by the pyrolysis of polycarbosilazane precursors: (Center director's Discretionary Fund final report). [Marshall Space Flight Center, Ala.]: National Aeronautics and Space Administration, George C. Marshall Space Flight Center, 1985.

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25

Albert, Tyler J., and Erik R. Swenson. The blood cells and blood count. Oxford University Press, 2016. http://dx.doi.org/10.1093/med/9780199600830.003.0265.

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Blood is a dynamic fluid consisting of cellular and plasma components undergoing constant regeneration and recycling. Like most physiological systems, the concentrations of these components are tightly regulated within narrow limits under normal conditions. In the critically-ill population, however, haematological abnormalities frequently occur and are largely due to non-haematological single- or multiple-organ pathology. Haematopoiesis originates from the pluripotent stem cell, which undergoes replication, proliferation, and differentiation, giving rise to cells of the erythroid, myeloid, and lymphoid series, as well as megakaryocytes, the precursors to platelets. The haemostatic system is responsible for maintaining blood fluidity and, at the same time, prevents blood loss by initiating rapid, localized, and appropriate blood clotting at sites of vascular damage. This system is complex, comprising both cellular and plasma elements, i.e. platelets, coagulation and fibrinolytic cascades, the natural intrinsic and extrinsic pathways of anticoagulation, and the vascular endothelium. A rapid, reliable, and inexpensive method of examining haematological disorders is the peripheral blood smear, which allows practitioners to assess the functional status of the bone marrow during cytopenic states. Red blood cells, which are primarily concerned with oxygen and carbon dioxide transport, have a normal lifespan of only 120 days and require constant erythropoiesis. White blood cells represent a summation of several circulating cell types, each deriving from the hematopoietic stem cell, together forming the critical components of both the innate and adaptive immune systems. Platelets are integral to haemostasis, and also aid our inflammatory and immune responses, help maintain vascular integrity, and contribute to wound healing.
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26

Trieloff, Mario. Noble Gases. Oxford University Press, 2017. http://dx.doi.org/10.1093/acrefore/9780190647926.013.30.

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This is an advance summary of a forthcoming article in the Oxford Encyclopedia of Planetary Science. Please check back later for the full article.Although the second most abundant element in the cosmos is helium, noble gases are also called rare gases. The reason is that they are not abundant on terrestrial planets like our Earth, which is characterized by orders of magnitude depletion of—particularly light—noble gases when compared to the cosmic element abundance pattern. Indeed, such geochemical depletion and enrichment processes make noble gases so versatile concerning planetary formation and evolution: When our solar system formed, the first small grains started to adsorb small amounts of noble gases from the protosolar nebula, resulting in depletion of light He and Ne when compared to heavy noble gases Ar, Kr, and Xe: the so-called planetary type abundance pattern. Subsequent flash heating of the first small mm to cm-sized objects (chondrules and calcium, aluminum rich inclusions) resulted in further depletion, as well as heating—and occasionally differentiation—on small planetesimals, which were precursors of larger planets and which we still find in the asteroid belt today from where we get rocky fragments in form of meteorites. In most primitive meteorites, we even can find tiny rare grains that are older than our solar system and condensed billions of years ago in circumstellar atmospheres of, for example, red giant stars. These grains are characterized by nucleosynthetic anomalies and particularly identified by noble gases, for example, so-called s-process xenon.While planetesimals acquired a depleted noble gas component strongly fractionated in favor of heavy noble gases, the sun and also gas giants like Jupiter attracted a much larger amount of gas from the protosolar nebula by gravitational capture. This resulted in a cosmic or “solar type” abundance pattern, containing the full complement of light noble gases. Contrary to Jupiter or the sun, terrestrial planets accreted from planetesimals with only minor contributions from the protosolar nebula, which explains their high degree of depletion and basically “planetary” elemental abundance pattern. Indeed this depletion enables another tool to be applied in noble gas geo- and cosmochemistry: ingrowth of radiogenic nuclides. Due to heavy depletion of primordial nuclides like 36Ar and 130Xe, radiogenic ingrowth of 40Ar by 40K decay, 129Xe by 129I decay, or fission Xe from 238U or 244Pu decay are precisely measurable, and allow insight in the chronology of fractionation of lithophile parent nuclides and atmophile noble gas daughters, mainly caused by mantle degassing and formation of the atmosphere.Already the dominance of 40Ar in the terrestrial atmosphere allowed C. F v. Weizsäcker to conclude that most of the terrestrial atmosphere originated by degassing of the solid Earth, which is an ongoing process today at mid ocean ridges, where primordial helium leaves the lithosphere for the first time. Mantle degassing was much more massive in the past; in fact, most of the terrestrial atmosphere formed during the first 100 million years of Earth´s history, and was completed at about the same time when the terrestrial core formed and accretion was terminated by a giant impact that also formed our moon. However, before that time, somehow also tiny amounts of solar noble gases managed to find their way into the mantle, presumably by solar wind irradiation of small planetesimals or dust accreting to Earth. While the moon-forming impact likely dissipated the primordial atmosphere, today´s atmosphere originated by mantle degassing and a late veneer with asteroidal and possibly cometary contributions. As other atmophile elements behave similar to noble gases, they also trace the origin of major volatiles on Earth, for example, water, nitrogen, sulfur, and carbon.
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