Quasi-Stellar Diameters and Intensity Fluctuations

Details Quasi-Stellar Diameters and Intensity Fluctuations Quasi-Stellar Diameters and Intensity Fluctuations

Aug 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964sci...145..918t&link_type=abstract

Science, Volume 145, Issue 3635, pp. 918-919

Physics

57

Scientific paper

It is shown there are relativistic limits on the fluctuations in
brightness which may be observed for a large spherical source, and also
for more general sources, so that quasi-stellar objects are probably no
more than light-days in size. There is thus a possibility that they may
be close to our galaxy.

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