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Browsing by Author "Busch, G."

Browsing by Author "Busch, G."

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  • 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 ...
  • 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 ...
  • 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 ...

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