A high Eddington-ratio, true Seyfert 2 galaxy candidate: Implications for broad-line region models
A bright, soft X-ray source was detected on 2010 July 14 during an XMM-Newton slew at a position consistent with the galaxy GSN 069 (z = 0.018). Previous ROSAT observations failed to detect the source and imply that GSN 069 is now ≥240 times brighter th
|Collections||ANU Research Publications|
|Source:||Monthly Notices of the Royal Astronomical Society|
|Access Rights:||Open Access|
|01_Miniutti_A_high_Eddington-ratio,_true_2013.pdf||922.9 kB||Adobe PDF|
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