Search Results - "Gaibler, V."

Jet-induced star formation in gas-rich galaxies by Gaibler, V., Khochfar, S., Krause, M., Silk, J.

“…Abstract Feedback from active galactic nuclei (AGN) has become a major component in simulations of galaxy evolution, in particular for massive galaxies. AGN…”
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Positive and negative feedback by AGN jets in high-redshift galaxies by Gaibler, V.

“…Simulations of feedback by jets from active galactic nuclei (AGN) in the past mostly focused on the interaction at large scales as the circumgalactic medium or…”
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Asymmetries in extragalactic double radio sources: clues from 3D simulations of jet-disc interaction by Gaibler, V., Khochfar, S., Krause, M.

“…Observational and theoretical studies of extragalactic radio sources have suggested that an inhomogeneous environment may be responsible for observed…”
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Very light magnetized jets on large scales – I. Evolution and magnetic fields by Gaibler, V., Krause, M., Camenzind, M.

“…Magnetic fields, which are undoubtedly present in extragalactic jets and responsible for the observed synchrotron radiation, can affect the morphology and…”
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Asymmetries in extragalactic double radio sources: clues from 3D simulations of jet-disc interaction: 3D jet-disc interaction by Gaibler, V., Khochfar, S., Krause, M.

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Very light magnetized jets on large scales - I. Evolution and magnetic fields by Gaibler, V., Krause, M., Camenzind, M.

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Very light magnetized jets on large scales – I. Evolution and magnetic fields: Very light magnetized jets by Gaibler, V., Krause, M., Camenzind, M.

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Positive and negative feedback by AGN jets in high-redshift galaxies by Gaibler, V

“…Simulations of feedback by jets from active galactic nuclei (AGN) in the past mostly focused on the interaction at large scales as the circumgalactic medium or…”
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Very Light Magnetized Jets on Large Scales - I. Evolution and Magnetic Fields by Gaibler, V, Krause, M, Camenzind, M

“…Magnetic fields, which are undoubtedly present in extragalactic jets and responsible for the observed synchrotron radiation, can affect the morphology and…”
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Large-scale Propagation of Very Light Jets in Galaxy Clusters by Gaibler, V, Camenzind, M, Krause, M

“…We performed MHD simulations of very light bipolar jets with density contrasts down to 10^-4 in axisymmetry, which were injected into a medium of constant…”
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