Self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics

Self-consistent bulge/disk/halo galaxy dynamical modeling using integral field kinematics

We introduce a method for modeling disk galaxies designed to take full advantage of data from integral field spectroscopy (IFS). The method fits equilibrium models to simultaneously reproduce the surface brightness, rotation, and velocity dispersion profiles of a galaxy. The models are fully self-co...

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Príomhchruthaitheoirí: Taranu, DS, Obreschkow, D, Dubinski, JJ, Fogarty, LMR, van de Sande, J, Catinella, B, Cortese, L, Moffett, A, Robotham, ASG, Allen, JT, Bland-Hawthorn, J, Bryant, JJ, Colless, M, Croom, SM, D'Eugenio, F, Davies, RL, Drinkwater, MJ, Driver, SP, Goodwin, M, Konstantopoulos, IS, Lawrence, JS, Lopez-Sanchez, AR, Lorente, NPF, Medling, AM, Mould, JR, Owers, MS, Power, C, Richards, SN, Tonini, C
Formáid: Journal article
Foilsithe / Cruthaithe: Institute of Physics 2017

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