The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
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Síða 9
... spectral type ( Secchi's second spectral 25 ' A new theory of the Milky Way ' , Ap . J. , xii ( 1900 ) . 26 Ap . J. , xxxvii ( 1913 ) 105 . type ) were generally found to have greater proper motions NINETEENTH - CENTURY ASTRONOMY : THE ...
... spectral type ( Secchi's second spectral 25 ' A new theory of the Milky Way ' , Ap . J. , xii ( 1900 ) . 26 Ap . J. , xxxvii ( 1913 ) 105 . type ) were generally found to have greater proper motions NINETEENTH - CENTURY ASTRONOMY : THE ...
Síða 95
... spectral shifts . He gave an expression for the de Sitter effect corresponding to ( 29 ) , 65 but this differs from ( 29 ) , not merely superficially . Eddington has one fewer power of sec ( r , / R ) on the right of his equation 70.4 ...
... spectral shifts . He gave an expression for the de Sitter effect corresponding to ( 29 ) , 65 but this differs from ( 29 ) , not merely superficially . Eddington has one fewer power of sec ( r , / R ) on the right of his equation 70.4 ...
Síða 139
... spectral displacements by the use of the classical Doppler formula . They avoided what would have amounted to a naïve definition of a velocity of recession , choosing to speak merely of spectra which would appear to indicate velocities ...
... spectral displacements by the use of the classical Doppler formula . They avoided what would have amounted to a naïve definition of a velocity of recession , choosing to speak merely of spectra which would appear to indicate velocities ...
Efni
COSMOLOGICAL DIFFICULTIES WITH | 16 |
FIELD THEORIES AND THE WISH TO | 24 |
The Le SageThomson explanation of gravitation | 38 |
Höfundarréttur | |
19 aðrir hlutar ekki sýndir
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The Measure of the Universe: A History of Modern Cosmology John David North Engin sýnishorn í boði - 1965 |
Common terms and phrases
absolute apparent magnitude appear argument assumption astronomical Bondi chapter clusters concept constant coordinates corresponding Cosmological Principle cosmological theories cosmologists covariant creation curvature density derived distance Eddington Einstein energy equivalent Euclidean Euclidean geometry example expanding universe expansion explained fact field equations finite formula function galactic galaxies geodesics geometry given gravitational field homogeneous Hubble Hubble's Hubble's Law hypothesis ibid idea infinite infinity interpretation isotropy Leibniz Lemaître light line-element Mach's Principle mass Math mathematical matter McCrea McVittie mean metric Milne Milne's motion nebulae Newton's Newtonian non-Euclidean geometry objects observer P. G. Tait parallax particles Phys physical possible problem radial reason regarded relation relativistic cosmology result Riemannian scientific seems sense simple Sitter solution space space-time spatial spectral spherical stars steady-state theories supposed tensor theoretical theory of gravitation Theory of Relativity tion Tolman universe velocity Weyl's Principle Whitehead Whitrow