期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 374, 期 3, 页码 1181-1184出版社
BLACKWELL PUBLISHING
DOI: 10.1111/j.1365-2966.2006.11238.x
关键词
galaxies : active; quasars : emission lines; quasars : general
By taking into account the relativistic corrections to the magnetic dipole operator, the theoretical [O-III] 5006.843/4958.911 line intensity ratio of 2.98 is obtained. In order to check this new value using the active galactic nuclei (AGN) spectra, we present the measurements of the flux ratio of the [O-III] lambda lambda 4959, 5007 emission lines for a sample of 62 AGN, obtained from the Sloan Digital Sky Survey (SDSS) data base and the published observations. We select only the high signal-to-noise ratio spectra for which the line shapes of the [O-III]lambda lambda 4959,5007 lines are the same. We obtained an averaged flux ratio of 2.993 +/- 0.014, which is in a good agreement with the theoretical one.
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