A high Eddington-ratio, true Seyfert 2 galaxy candidate: Implications for broad-line region models
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Miniutti, G
Saxton, R.
Rodriguez-Pascual, P M
Read, A M
Esquej, P
Colless, Matthew
Dobbie, P
Spolaor, M
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Blackwell Publishing Ltd
Abstract
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
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Monthly Notices of the Royal Astronomical Society
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Restricted until
2037-12-31
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