A theoretical explanation for the Central Molecular Zone asymmetry
Sormani, M Tress, R Ridley, M Glover, S Klessen, R Binney, J Magorrian, J Smith, R (12 Jul 2017) doi:10.48550/arxiv.1707.03650
Orbit-superposition models of discrete, incomplete stellar kinematics: application to the Galactic centre
Magorrian, J (16 Sep 2018) doi:10.48550/arxiv.1809.05946
The Demography of Massive Dark Objects in Galaxy Centres
Magorrian, J Tremaine, S Richstone, D Bender, R Bower, G Dressler, A Faber, S Gebhardt, K Green, R Grillmair, C Kormendy, J Lauer, T (07 Aug 1997) doi:10.48550/arxiv.astro-ph/9708072
The slope of the black-hole mass versus velocity dispersion correlation
Tremaine, S Gebhardt, K Bender, R Bower, G Dressler, A Faber, S Filippenko, A Green, R Grillmair, C Ho, L Kormendy, J Lauer, T Magorrian, J Pinkney, J Richstone, D (26 Mar 2002) doi:10.48550/arxiv.astro-ph/0203468
Generating Equilibrium Dark Matter Halos: Inadequacies of the Local Maxwellian Approximation
Kazantzidis, S Magorrian, J Moore, B (18 Sep 2003) doi:10.48550/arxiv.astro-ph/0309517
The Centers of Early-Type Galaxies with HST. V. New WFPC2 Photometry
Lauer, T Faber, S Gebhardt, K Richstone, D Tremaine, S Ajhar, E Aller, M Bender, R Dressler, A Filippenko, A Green, R Grillmair, C Ho, L Kormendy, J Magorrian, J Pinkney, J Siopis, C (01 Dec 2004) doi:10.48550/arxiv.astro-ph/0412040
The Masses of Nuclear Black Holes in Luminous Elliptical Galaxies and Implications for the Space Density of the Most Massive Black Holes
Lauer, T Faber, S Richstone, D Gebhardt, K Tremaine, S Postman, M Dressler, A Aller, M Filippenko, A Green, R Ho, L Kormendy, J Magorrian, J Pinkney, J (29 Jun 2006) doi:10.48550/arxiv.astro-ph/0606739
Evidence of a Supermassive Black Hole in the Galaxy NGC 1023 from the Nuclear Stellar Dynamics
Bower, G Green, R Bender, R Gebhardt, K Lauer, T Magorrian, J Richstone, D Danks, A Gull, T Hutchings, J Joseph, C Kaiser, M Weistrop, D Woodgate, B Nelson, C Malumuth, E (09 Nov 2000) doi:10.48550/arxiv.astro-ph/0011204
Black Hole Mass Determinations From Orbit Superposition Models are Reliable
Richstone, D Gebhardt, K Aller, M Bender, R Bower, G Dressler, A Faber, S Filippenko, A Green, R Ho, L Kormendy, J Lauer, T Magorrian, J Pinkney, J Siopis, C Tremaine, S (10 Mar 2004) doi:10.48550/arxiv.astro-ph/0403257
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