Other
Scientific paper
Aug 1967
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967natur.215..605g&link_type=abstract
Nature, Volume 215, Issue 5101, pp. 605-606 (1967).
Other
16
Scientific paper
IT has been suggested1 that the optical variability of the quasi-stellar source 3C 273 is compatible with a model of a quasar which is a complex of several sources of the same type; for example, a star cluster within which there are independent occasional collisions and possibly flash-like supernovae as well. This claim is incorrect. In fact, the statistical properties of the optical variability of 3C 273 are such as to suggest that the separate parts of a quasar nucleus interact with each other. In other words, a quasar nucleus is in the limit of a single body2.
Chertoprud V. E.
Gudzenko L. I.
Ozernoy Leonid M.
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