White, Glenn J. and Ricketts, Martin J.
(1979).
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| URL: | http://adsabs.harvard.edu/abs/1979MNRAS.187..757W |
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Abstract
Observations of the quasar 3C273 made during 1975-77 have shown that the X-ray flux varied on a time scale of several months. No similar variation was present in radio and optical data taken at similar times. If this variation results from luminosity variations of a central compact object, then an upper limit of ≤4 x 1017cm can be set on its dimensions.
| Item Type: | Journal Article |
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| Copyright Holders: | 1979 Royal Astronomical Society |
| ISSN: | 0035-8711 |
| Keywords: | light curve; quasars; statistical analysis; x-ray astronomy; Compton effect; luminous intensity; stellar luminosity |
| Academic Unit/Department: | Science > Physical Sciences |
| Interdisciplinary Research Centre: | Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR) |
| Item ID: | 33275 |
| Depositing User: | Glenn White |
| Date Deposited: | 28 Mar 2012 13:30 |
| Last Modified: | 29 Mar 2012 16:04 |
| URI: | http://oro.open.ac.uk/id/eprint/33275 |
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