Fig. 3 from An Accreting Black Hole in the Nuclear Star Cluster of the Bulgeless Galaxy NGC 1042

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An Accreting Black Hole in the Nuclear Star Cluster of the Bulgeless Galaxy NGC 1042

Authors: Joseph C. Shields, C. Jakob Walcher, Torsten Böker, Luis C. Ho, Hans-Walter Rix, and Roeland P. van der Marel

Shields et al. 2008 The Astrophysical Journal 682 104.

Provider: AAS Journals

Caption: Fig. 3.

Normalized emission profiles measured in the center of NGC 1042 for [N II] λ6583 (dashed line) and Hα (dotted line) after subtraction of a constant continuum level. The residual Hα profile after subtraction of a model stellar continuum is shown by the solid line.

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