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This annually updated and comprehensive guide helps students and parents compare colleges within a specific geographic area (New York). Accredited regional colleges and universities are profiled with the latest information on financial aid, admissions, and student body statistics.
The latest volume in this respected series encompasses subjects as diverse as materials with optical or biological properties, chiral molecules, advanced physical methods in organic synthesis and non-classical synthetic methodologies. Critical surveys are presented on: total synthesis of natural products; organometallic compounds in organic synthesis; the introduction and transformation of functional groups; and solid supported synthesis. The accompanying CD-ROM provides pdf files of the articles included in the book. This volume will be an invaluable reference source for students and researchers in both academia and industry.
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This work contains over thirty chapters by leading researchers in the field of oxidative biology, originally presented as articles in an extended Forum in the highly-cited journal, Free Radical Biology & Medicine. The papers in this Forum (or Symposium-in-print) spanned seven issues of the journal, over many months. This is the first time that all of these expert contributions are presented in one place.Reliable methods for measuring OSS in organisms are essential. These would, amongst other things, offer applications as early warning signals for cancer and heart disease - eventually giving a range of measurable oxidation products best related to any given disease state.Additional observations relevant to OSS include: how much do measures of OSS vary in a group of humans? Does OSS decrease as a result of life-change factors and does it increase with age? With disease? With stress? Can a non-invasive, reliable, reputable measure of OSS be identified?This informative book provides the reader with the latest status of studies into OSS, currently used examples of BOSS, and answers to at least some of the questions posed above.
All galaxies host a super-massive black hole in their center. These black holes grow their mass in symbiosis with their host galaxy and moderate their star formation. When matter is driven towards the nucleus, an accretion disk is formed to transfer angular momentum and considerable energy is released when the material falls into the black hole: this is the phenomenon of active galactic nuclei (AGN). A nucleus can shine one thousand times more brightly than the entire galaxy with its 200 billion stars. The nuclear activity can take many forms, from very powerful quasars to more ordinary Seyfert galaxies, passing by radio-galaxies, which eject a collimated plasma at ten times the radius of the galaxy. This book examines all of these manifestations and presents a unified view. When two galaxies merge, a binary black hole is formed and the two black holes will spiral inwards and merge, emitting long gravitational waves, which could be detected by the future LISA satellite.
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