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Browsing by Author "Davis, T. A."

Browsing by Author "Davis, T. A."

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  • The Close AGN Reference Survey (CARS). A massive multi-phase outflow impacting the edge-on galaxy HE 1353-1917 
    Husemann, B.; Scharwächter, J.; Davis, T. A.; Pérez-Torres, M.; Smirnova-Pinchukova, I.; Tremblay, Grant R.; Krumpe, M.; Combes, F.; Baum, S. A.; Busch, G.; Connor, T.; Croom, S. M.; Gaspari, M.; Kraft, Ralph P.; O'Dea, C. P.; Powell, M.; Singha, M.; Urrutia, T. (2019)
    Context. Galaxy-wide outflows driven by star formation and/or an active galactic nucleus (AGN) are thought to play a crucial rule in the evolution of galaxies and the metal enrichment of the inter-galactic medium. Direct ...
  • The Close AGN Reference Survey (CARS). Comparative analysis of the structural properties of star-forming and non-star-forming galaxy bars 
    Neumann, J.; Gadotti, D. A.; Wisotzki, L.; Husemann, B.; Busch, G.; Combes, F.; Croom, S. M.; Davis, T. A.; Gaspari, M.; Krumpe, M.; Pérez-Torres, M. A.; Scharwächter, J.; Smirnova-Pinchukova, I.; Tremblay, Grant R.; Urrutia, T. (2019)
    The absence of star formation in the bar region that has been reported for some galaxies can theoretically be explained by shear. However, it is not clear how star-forming (SF) bars fit into this picture and how the dynamical ...
  • The Close AGN Reference Survey (CARS). Discovery of a global [C II] 158 µm line excess in AGN HE 1353-1917 
    Smirnova-Pinchukova, I.; Husemann, B.; Busch, G.; Appleton, P.; Bethermin, M.; Combes, F.; Croom, S.; Davis, T. A.; Fischer, C.; Gaspari, M.; Groves, B.; Klein, R.; O'Dea, C. P.; Pérez-Torres, M.; Scharwächter, J.; Singha, M.; Tremblay, Grant R.; Urrutia, T. (2019)
    The [C II]?158 µm line is one of the strongest far-infrared (FIR) lines and an important coolant in the interstellar medium of galaxies that is accessible out to high redshifts. The excitation of [C II] is complex and can ...
  • The Close AGN Reference Survey (CARS). IFU survey data and the BH mass dependence of long-term AGN variability 
    Husemann, B.; Singha, M.; Scharwächter, J.; McElroy, R.; Neumann, J.; Smirnova-Pinchukova, I.; Urrutia, T.; Baum, S. A.; Bennert, V. N.; Combes, F.; Croom, S. M.; Davis, T. A.; Fournier, Y.; Galkin, A.; Gaspari, M.; Enke, H.; Krumpe, M.; O'Dea, C. P.; Pérez-Torres, M.; Rose, T.; Tremblay, G. R.; Walcher, C. J. (2022)
    Context. Active galactic nuclei (AGN) are thought to be intimately connected with their host galaxies through feeding and feedback processes. A strong coupling is predicted and supported by cosmological simulations of ...
  • The Close AGN Reference Survey (CARS). Locating the [O III] wing component in luminous local Type 1 AGN 
    Singha, M.; Husemann, B.; Urrutia, T.; O'Dea, C. P.; Scharwächter, J.; Gaspari, M.; Combes, F.; Nevin, Rebecca; Terrazas, Bryan A.; Pérez-Torres, M.; Rose, T.; Davis, T. A.; Tremblay, G. R.; Neumann, J.; Smirnova-Pinchukova, I.; Baum, S. A. (2022)
    Context. The strong asymmetry in the optical [O III] λ5007 emission line is one of the best signatures of active galactic nuclei (AGN) driven warm (∼10<SUP>4</SUP> K) ionized gas outflows on host galaxy scales. While ...
  • The Close AGN Reference Survey (CARS). No obvious signature of AGN feedback on star formation, but subtle trends 
    Smirnova-Pinchukova, I.; Husemann, B.; Davis, T. A.; Smith, C. M. A.; Singha, M.; Tremblay, G. R.; Klessen, R. S.; Powell, M.; Connor, T.; Baum, S. A.; Combes, F.; Croom, S. M.; Gaspari, M.; Neumann, J.; O'Dea, C. P.; Pérez-Torres, M.; Rosario, D. J.; Rose, T.; Scharwächter, J.; Winkel, N. (2022)
    Context. Active galactic nuclei (AGN) are thought to be responsible for the suppression of star formation in massive ∼10<SUP>10</SUP> M<SUB>⊙</SUB> galaxies. While this process is a key feature in numerical simulations ...
  • The Close AGN Reference Survey (CARS). Tracing the circumnuclear star formation in the super-Eddington NLS1 Mrk 1044 
    Winkel, N.; Husemann, B.; Davis, T. A.; Smirnova-Pinchukova, I.; Bennert, V. N.; Combes, F.; Gaspari, M.; Jahnke, K.; Neumann, J.; O'Dea, C. P.; Pérez-Torres, M.; Singha, M.; Tremblay, G. R.; Rix, H. W. (2022)
    Context. The host galaxy conditions for rapid supermassive black hole growth are poorly understood. Narrow-line Seyfert 1 (NLS1) galaxies often exhibit high accretion rates and are hypothesized to be prototypes of active ...

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