Optical Variability of a Bright New Quasi-stellar Source

Details Optical Variability of a Bright New Quasi-stellar Source Optical Variability of a Bright New Quasi-stellar Source

Aug 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971natur.232..622l&link_type=abstract

Nature, Volume 232, Issue 5313, pp. 622-623 (1971).

Physics

9

Scientific paper

BROWNE1 has identified the radio source 1215 + 30 of the Bologna B2 survey with a remarkably bright quasi-stellar source of magnitude approximately 14.5. We report here that its optical flux is variable by more than two magnitudes, with discernible brightness changes over time scales of hours, as well as secular trends on a time scale of years.

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