Gravitational Multipole Radiation

Previous article Next article Gravitational Multipole RadiationJon MathewsJon Mathewshttps://doi.org/10.1137/0110059PDFPDF PLUSBibTexSections ToolsAdd to favoritesExport CitationTrack CitationsEmail SectionsAbout[1] A. Einstein, Théorie de la Relativité, Hermann et Cie, Paris, 1933 Google Scholar[2] H. Weyl, Space-Time-Matter, Dover Publications Inc., New York, 1950, 315–317 0044.22704 Google Scholar[3] Albert Einstein, The meaning of relativity. Third edition, revised, including The Generalized Theory of Gravitation, Princeton University Press, Princeton, N. J., 1950, 106– MR0048945 0037.42005 Google Scholar[4] A. Einstein, Théorie de la Relativité, Hermann et Cie, Paris, 1933, 106– Google Scholar[5] P. A. Schlipp, Albert Einstein: Philosopher-Scientist, The Library of Living Philosophers, Inc., Evanston, Ill., 1949, 481– MR0035229 0038.14804 Google Scholar[6] A. Einstein, Théorie de la Relativité, Hermann et Cie, Paris, 1933, 99–109 Google Scholar[7] G. C. McVittie, Fact and Theory in Cosmology, Eyre and Spottiswoode, London, 1961 0105.21304 Google Scholar[8] M. L. Humason, , N. U. Mayall and , A. R. Sandage, Redshifts and magnitudes of extragalactic nebulae, Astr. J., 61 (1956), 97– 10.1086/107297 CrossrefISIGoogle Scholar[9] F. Hoyle and , A. R. Sandage, The second-order term in the redshift-magnitude relation, Publ. Astr. Soc. Pacific, 68 (1956), 301– 10.1086/126942 CrossrefISIGoogle Scholar[10] W. A. Baum, Photoelectric determinations of redshifts beyond 0.2c, Astr. J., 62 (1957), 6–, W. A. Baum and R. Minkowski, Observations of a large red-shift, Astr. J., 65 (1960), p. 483 10.1086/107433 CrossrefISIGoogle Scholar[11] Allan Sandage, The light travel time and the evolutionary correction to magnitudes of distant galaxies, Astrophys. J., 134 (1961), 916–926 10.1086/147218 MR0135164 CrossrefISIGoogle Scholar[12] Th. Schmidt-Kaler, On the age of the galaxy and the helium content of the old population I stars, Observatory, 81 (1961), 226– Google Scholar[13] J. H. Oort, La Structure et l'Evolution de l'Univers, Stoops, Brussels, 1958, 163– Google Scholar[14] A. R. Sandage, The ability of the 200-inch telescope to discriminate between selected world models, Astrophys. J., 133 (1961), 355– 10.1086/147041 CrossrefISIGoogle Scholar[15] N. J. Woolf, Age of Messier 3, Astr. J., 67 (1962), 286– 10.1086/108865 CrossrefISIGoogle Scholar Previous article Next article FiguresRelatedReferencesCited ByDetails Volume 10, Issue 4| 1962Journal of the Society for Industrial and Applied Mathematics569-801 History Published online:13 July 2006 InformationCopyright © 1962 Society for Industrial and Applied MathematicsPDF Download Article & Publication DataArticle DOI:10.1137/0110059Article page range:pp. 768-780ISSN (print):0368-4245ISSN (online):2168-3484Publisher:Society for Industrial and Applied Mathematics