IPAC Astronomy Lunch Seminar
Recent Herschel/PACS observations have detected massive amounts of molecular gas gusting at high velocities - in some cases in excess of 1000 kilometres per second - from the centres of a set of merging galaxies. Driven by star formation and central black holes, these powerful storms are strong enough to sweep away billions of solar masses of molecular gas and to interfere with global galactic processes. These observations indicate that, in the galaxies hosting the brightest Active Galactic Nuclei, outflows can clear the entire supply for creating stars and feeding the black hole. This finding provides long-sought-after evidence of highly energetic feedback processes taking place in galaxies as they evolve. I will summarize the current status of this project, which is part of the Herschel Guaranteed Time Key Project SHINING. In case enough pizza is provided I will also summarize further SHINING results which help to understand the different modes of star formation (major merger vs. steady accretion) in the early universe.
For more information, please contact Luisa Rebull by phone at x4565 or by email at [email protected] or visit http://www.ipac.caltech.edu/events.
Event Series
IPAC Astronomy Lunch Seminar Series