Figure 10 from The Next Generation Fornax Survey (NGFS). IV. Mass and Age Bimodality of Nuclear Clusters in the Fornax Core Region

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The Next Generation Fornax Survey (NGFS). IV. Mass and Age Bimodality of Nuclear Clusters in the Fornax Core Region

Authors: Yasna Ordenes-Briceño, Thomas H. Puzia, Paul Eigenthaler, Matthew A. Taylor, Roberto P. Muñoz, Hongxin Zhang, Karla Alamo-Martínez, Karen X. Ribbeck, Eva K. Grebel, Simón Ángel, Patrick Côté, Laura Ferrarese, Michael Hilker, Ariane Lançon, Steffen Mieske, Bryan W. Miller, Yu Rong, and Ruben Sánchez-Janssen

2018 The Astrophysical Journal 860 4.

Provider: AAS Journals

Caption: Figure 10.

Top panel: nucleus vs. host galaxy stellar mass for different subsets of nucleated NGFS galaxies and other galaxies from the literature. The SMBH mass vs. galaxy mass relation from McConnell & Ma (2013) is shown with 1σ and 3σ limits as dashed-line and shaded regions, respectively. Bottom panel: nucleus-to-galaxy mass ratio (﹩{\eta }_{n}={{ \mathcal M }}_{\mathrm{nuc}}/{{ \mathcal M }}_{\mathrm{gal}}﹩) vs. galaxy mass. We approximate the ETG data with a bi-regime fit for which the slopes of the low-mass and high-mass galaxy masses are labeled.

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