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Titlebook: Examining the Big Bang and Diffuse Background Radiations; Menas Kafatos,Yoji Kondo Book 1996 International Astronomical Union 1996 Gravity

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书目名称Examining the Big Bang and Diffuse Background Radiations
编辑Menas Kafatos,Yoji Kondo
视频video
丛书名称International Astronomical Union Symposia
图书封面Titlebook: Examining the Big Bang and Diffuse Background Radiations; Menas Kafatos,Yoji Kondo Book 1996 International Astronomical Union 1996 Gravity
描述IAU Symposium No. 168, .Examining the Big Bang and DiffuseBackground. .Radiations., took place on August 23-26,1994 at the XXIInd IAU General Assembly in the Hague, Netherlands..The meeting attracted a large number - over 250 - ofastronomers, reflecting the strong interest engendered by the greatadvances in cosmology made in recent years. There is still a multitudeof unresolved problems in modern cosmology and the symposium offered awonderful occasion to examine them objectively, at a place where manyleading workers in related fields gathered together. .After the introduction by IAU President L. Woltjer and the historicalbackground by Vice Present Virginia Trimble, the volume begins withreviews of the cosmic microwave radiation from COBE (Cosmic BackgroundExplorer). Reviews of recent observations then extend from radio toinfrared, visible light, ultraviolet, X-rays and gamma-rays. It isfollowed by theoretical models for the Big Bang and Inflation, andalternative views to the Big Bang. Following a discourse on Probes andFuture Tests, the meeting ended with a Panel Discussion on `MajorUnsolved Problems of Cosmology‘. Some forty-four contributed papers- both oral and poster reports -
出版日期Book 1996
关键词Gravity; Inflation; Redshift; active galactic nuclei; cosmic microwave background; cosmology; deep-sky; gra
版次1
doihttps://doi.org/10.1007/978-94-009-0145-2
isbn_softcover978-0-7923-3815-4
isbn_ebook978-94-009-0145-2Series ISSN 1743-9213 Series E-ISSN 2352-2186
issn_series 1743-9213
copyrightInternational Astronomical Union 1996
The information of publication is updating

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Measurement and Implications of the Cosmic Microwave Background Spectrumhe early universe. It also measured emission from nearby sources such as the stars, dust, molecules, atoms, ions, and electrons in the Milky Way, and dust and comets in the Solar System. It was launched 18 November 1989 on a Delta rocket., carrying one microwave instrument and two cryogenically cool
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Fluctuations In The Microwave Skyw have secure detections on some angular scales and improved upper limits on others. As the sensitivity of such searches increases, understanding sources of foreground noise (e.g., Galactic and extragalactic radio emission) becomes more important. Also reviewed are the contributions aperture synthes
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The Cobe Dirbe Search for the Cosmic Infrared Backgroundotropic cosmic infrared background radiation over the spectral range from 1.25 to 240 µm. The cumulative emissions of pregalactic, protogalactic, and evolving galactic systems are expected to be recorded in this background. The DIRBE instrument has mapped the full sky with high redundancy at solar e
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Degree Scale Anisotropy: Current Statusation of structure we now observe. Recent advances in degree scale anisotropy measurements have allowed us to begin critically testing cosmological models. Combined with the larger scale measurements from COBE we are now able to directly compare data and theory. These measurements promise future pro
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Galaxy Motions in The Nearby Universeof the field is that (1) convincing infall has been detected into dense clusters, especially the Virgo cluster, (2) the microwave background direction is moderately well aligned with the measured flow nearby but not apparently on larger scales, and (3) there is good but not perfect consistency betwe
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