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Titlebook: Supermassive Black Holes in the Distant Universe; Amy J. Barger Book 2004 Springer Science+Business Media B.V. 2004 Accretion.Galaxy.Obser

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Modeling the Accretion History of Supermassive Black Holes,se remnant black holes from the stellar kinematics of local galaxies and the quasar phenomenon at high redshifts point to the presence of assembled SMBHs. The accretion history of SMBHs can be reconstructed using observations at high and low redshifts as model constraints. Observations of galaxies a
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The Formation and Evolution of the First Massive Black Holes,These black holes grow by mergers and gas accretion, evolve into the population of bright quasars observed at lower redshifts, and eventually leave the supermassive black hole remnants that are ubiquitous at the centers of galaxies in the nearby universe. The astrophysical processes responsible for
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Distant X-Ray Galaxies: Insights from the Local Population,tunately, distant X-ray galaxies tend to be very faint at all wavelengths, which hinders efforts to perform this census. This chapter discusses the insights that can be obtained through comparison of the distant population to local X-ray galaxies, whose properties are well characterized. Such compar
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n source of calories for the diets of 800 million people in Africa, South America, and Southeast Asia. Over the past 20 years, the Brazilian Agricultural Research Corporation (Embrapa) and collaborators have been developing innovations for the use and postharvest processing of cassava. These technol
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Laura Ferrarese start of the XW epidemic, complete uprooting of diseased mats (CMU) was recommended. There was little adoption of CMU, especially by women farmers, because it was labor-intensive and it sacrificed banana production for up to 2 years. CMU assumed that infection on a single plant would systemically s
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