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Ionized gas kinematics of massive elliptical galaxies in CALIFA and in cosmological zoom-in simulations
- Source :
- Florian , J , Ziegler , B , Hirschmann , M , Papaderos , P , Choi , E , Frigo , M , Gomes , J-M & Somerville , R S 2020 , ' Ionized gas kinematics of massive elliptical galaxies in CALIFA and in cosmological zoom-in simulations ' , Astronomy & Astrophysics , vol. 635 , A41 .
- Publication Year :
- 2020
-
Abstract
- Context. Powerful active galactic nuclei (AGN) are supposed to play a key regulatory role on the evolution of their host galaxies by shaping the thermodynamic properties of their gas component. However, little is known as to the nature and the visibility timescale of the kinematical imprints of AGN-driven feedback. Gaining theoretical and observational insights into this subject is indispensable for a thorough understanding of the AGN-galaxy coevolution and could yield empirical diagnostics for the identification of galaxies that have experienced a major AGN episode in the past.Aims. We present an investigation of kinematical imprints of AGN feedback on the warm ionized gas medium (WIM) of massive early-type galaxies (ETGs). To this end, we take a two-fold approach that involves a comparative analysis of H alpha velocity fields in 123 local ETGs from the CALIFA (Calar Alto Legacy Integral Field Area Survey) integral field spectroscopy survey with 20 simulated galaxies from high-resolution hydrodynamic cosmological SPHgal simulations. The latter were resimulated for two modeling setups, one with and another without AGN feedback.Methods. In order to quantify the effects of AGN feedback on gas kinematics, we measured three parameters that probe deviations from simple regular rotation by using the kinemetry package. These indicators trace the possible presence of distinct kinematic components in Fourier space (k(3,& x2006;5)/k(1)), variations in the radial profile of the kinematic major axis (sigma(PA)), and offsets between the stellar and gas velocity fields (Delta phi). These quantities were monitored in the simulations from a redshift 3 to 0.2 to assess the connection between black hole accretion history, stellar mass growth, and the kinematical perturbation of the WIM.Results. Observed local massive galaxies show a broad range of irregularities, indicating disturbed warm gas motions, which is irrespective of being classified via diagnosti
Details
- Database :
- OAIster
- Journal :
- Florian , J , Ziegler , B , Hirschmann , M , Papaderos , P , Choi , E , Frigo , M , Gomes , J-M & Somerville , R S 2020 , ' Ionized gas kinematics of massive elliptical galaxies in CALIFA and in cosmological zoom-in simulations ' , Astronomy & Astrophysics , vol. 635 , A41 .
- Notes :
- application/pdf, English
- Publication Type :
- Electronic Resource
- Accession number :
- edsoai.on1322747761
- Document Type :
- Electronic Resource