The Measure of the Universe: A History of Modern CosmologyClarendon Press, 1965 - 436 síður |
From inside the book
Niðurstöður 1 - 3 af 6
Síða 247
... magnitude need not be accurately known : but most of the immense practical ... apparent magnitudes not greater than m , and m , was given for relativistic ... magnitude of these sources can be decided . ( iii ) The number of the sources ...
... magnitude need not be accurately known : but most of the immense practical ... apparent magnitudes not greater than m , and m , was given for relativistic ... magnitude of these sources can be decided . ( iii ) The number of the sources ...
Síða 379
... apparent magnitude less than 20-3 ' . The members of the class might just as well be named and listed . In the case of the ' infinite whole ' there is no possibility of a definition by extension . But that is no reason why an ...
... apparent magnitude less than 20-3 ' . The members of the class might just as well be named and listed . In the case of the ' infinite whole ' there is no possibility of a definition by extension . But that is no reason why an ...
Síða 420
... apparent magnitude ( all magnitudes given below are photographic ) —can be found granted only a great deal of information as to the area , the temperature , the spectral distribution function of the source , and the so - called ...
... apparent magnitude ( all magnitudes given below are photographic ) —can be found granted only a great deal of information as to the area , the temperature , the spectral distribution function of the source , and the so - called ...
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
Aðrar útgáfur - View all
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