000 | 03096nam a22005655i 4500 | ||
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001 | 978-3-540-47296-4 | ||
003 | DE-He213 | ||
005 | 20160624101852.0 | ||
007 | cr nn 008mamaa | ||
008 | 121227s1992 gw | s |||| 0|eng d | ||
020 |
_a9783540472964 _9978-3-540-47296-4 |
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024 | 7 |
_a10.1007/3-540-55842-X _2doi |
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050 | 4 | _aQB4 | |
072 | 7 |
_aPG _2bicssc |
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072 | 7 |
_aSCI004000 _2bisacsh |
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072 | 7 |
_aNAT033000 _2bisacsh |
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082 | 0 | 4 |
_a520 _223 |
245 | 1 | 0 |
_aNew Insights into the Universe _h[electronic resource] : _bProceeding of a Summer School Held in València, Spain 23–27 September 1991 / _cedited by Vincent J. Martínez, Miquel Portilla, Diego Sáez. |
260 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1992. |
|
264 | 1 |
_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg, _c1992. |
|
300 |
_aXI, 300 p. _bonline resource. |
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336 |
_atext _btxt _2rdacontent |
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337 |
_acomputer _bc _2rdamedia |
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338 |
_aonline resource _bcr _2rdacarrier |
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347 |
_atext file _bPDF _2rda |
||
490 | 1 |
_aLecture Notes in Physics, _x0075-8450 ; _v408 |
|
505 | 0 | _aStatistics of cosmological density fields -- Large-scale structures and motions: Linear theory and statistics -- Clusters of galaxies as probes for the large scale structure -- Galaxy formation with gravitation, hydrodynamics and active star formation -- Secondary anisotropies in the CMB -- The Relikt missions: Results and prospects to detect the microwave background anisotropy -- ROSAT observations of clusters of galaxies -- Statistics of gravitational lensing 1: Strong lenses -- Statistics of gravitational lensing 2: Weak lenses. | |
520 | _aIndispensable for the building of cosmological models are precise observational data. To provide such data is the main purpose of this book. First, an analysis of recent cosmological observations using artificial satellites and large ground-based telescopes is given. Among these are the observation of the spatial distribution of galaxies and clusters, the detection of peculiar velocity fields in large regions, and the measurement of anisotropies in the microwave background radiation. Second, the authors present theoretical models which best fit the given observational data. The book addresses graduate students and astronomers and astrophysicists. | ||
650 | 0 | _aPhysics. | |
650 | 0 | _aPhysical geography. | |
650 | 0 | _aAstronomy. | |
650 | 0 | _aAstrophysics. | |
650 | 0 | _aRelativity (Physics). | |
650 | 1 | 4 | _aPhysics. |
650 | 2 | 4 | _aAstronomy. |
650 | 2 | 4 | _aAstrophysics. |
650 | 2 | 4 | _aGeophysics/Geodesy. |
650 | 2 | 4 | _aRelativity and Cosmology. |
700 | 1 |
_aMartínez, Vincent J. _eeditor. |
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700 | 1 |
_aPortilla, Miquel. _eeditor. |
|
700 | 1 |
_aSáez, Diego. _eeditor. |
|
710 | 2 | _aSpringerLink (Online service) | |
773 | 0 | _tSpringer eBooks | |
776 | 0 | 8 |
_iPrinted edition: _z9783540558422 |
786 | _dSpringer | ||
830 | 0 |
_aLecture Notes in Physics, _x0075-8450 ; _v408 |
|
856 | 4 | 0 | _uhttp://dx.doi.org/10.1007/3-540-55842-X |
942 |
_2EBK2618 _cEBK |
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999 |
_c31912 _d31912 |