Fig. 4 from A Log‐Quadratic Relation for Predicting Supermassive Black Hole Masses from the Host Bulge Sérsic Index

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A Log‐Quadratic Relation for Predicting Supermassive Black Hole Masses from the Host Bulge Sérsic Index

Authors: Alister W. Graham and Simon P. Driver

Graham & Driver 2007 The Astrophysical Journal 655 77.

Provider: AAS Journals

Caption: Fig. 4.

Predicted correlation between SMBH mass and the central B‐band surface brightness of the host bulge, after allowing for excess nuclear flux and partially depleted cores, as mentioned in § 6. The solid line corresponds to eq. (9), and the dashed line corresponds to eq. (10).

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