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An Hα Dynamical Mass for HE 0047–1756
2009
Proceedings of the International Astronomical Union
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AbstractWe derive Mbulge for HE 0047–1756 via Hα gas dynamics. The resulting large value of MBH/Mbulge may imply evolution in the correlation at high redshifts.
doi:10.1017/s1743921310006253
fatcat:cv6eaclcmrbnnknmae3nxb3vqe