PowerPoint Presentation Deep fields with MUSE Simon Lilly (ETH Zurich) with Sebastiano Cantalupo (UCSC) and the MUSE Consortium 20143D ESO March 14 2014 1 “quenched”…
The cooling-flow problem Bremsstrahlung emission ) L / n2 ) center parts cool faster. Pressure equilibrium ) mass in-flow ) density increases. Mariano Mendez - SRON The cooling-flow…
The Fate of the X-Ray Emitting Gas in the Early-Type Galaxy NGC 5044 O’Sullivan Jeremy Lim William Forman Jan Vrtilek Christine Jones Ewan O’Sullivan Francoise Combes…
PowerPoint Presentation Deep fields with MUSE Simon Lilly (ETH Zurich) with Sebastiano Cantalupo (UCSC) and the MUSE Consortium 20143D ESO March 14 2014 1 “quenched”…
The cooling-flow problem Bremsstrahlung emission ) L / n2 ) center parts cool faster. Pressure equilibrium ) mass in-flow ) density increases. Mariano Mendez - SRON The cooling-flow…
Properties of the NLR from Spatially Resolved Spectroscopy Nicola Bennert University of California Riverside Collaborators: Bruno Jungwiert, Stefanie Komossa, Martin Haas,…