Interstellar Medium


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The Interstellar Medium of High Redshift Galaxies

9 April - 4 May 2018
Andrea Ferrara, Richard Ellis, Fabian Walter



In the last decade the search for galaxies seen within the reionisation era, a period from 500 Myr to approximately 1Gyr after the Big Bang when the Universe transitioned from a neutral to ionised form, has been extremely successful. Exploiting both ground-based (VLT, Keck, Subaru) and space-borne (HST, Spitzer) telescopes, about 1500 galaxies have been discovered in the relevant redshift interval 6 < z < 11. 

Deep surveys have provided valuable demographic data for these early galaxies. They have also provided an initial characterisation of the stellar component, in terms of star formation rates, masses, sizes, etc.  However, to be truly successful such effort must be complemented with information about the internal structure and interstellar medium (ISM) of early galaxies, whose properties are currently unknown.

The ISM plays a fundamental role in galaxy evolution. The diffuse ISM contains the material from which molecular clouds, and thus ultimately stars, form. The Interstellar Radiation Field (ISRF), cosmic rays, and magnetic fields permeate it. By absorbing and radiating the energy produced by stars, it acts as an energy regulator for the galaxy thus playing a pivotal role in galaxy evolution. The ISM is also a repository of metals and dust, which in turn produce emission lines and continuum radiation that represent valuable probes of the physics of early star formation, chemical enrichment and the ionising radiation field.

The key questions we propose to address at this MIAPP programme are concerned with the properties, structure and evolution of the interstellar medium of high redshift galaxies in the context of cosmic reionisation. These include the following:

  • How do early galaxies acquire their mass? Are cold flows ubiquitous at high redshift?
  • How does the gaseous content of galaxies evolve with cosmic time?
  • What about gas kinematics? Can we use it to reliably measure dynamical masses?
  • Is the ISM porous enough to allow the escape of ionising photons in the intergalactic medium?
  • When and how do galaxies get enriched with heavy elements and dust?
  • What physics regulates the interplay between the galaxy and its circumgalactic medium?
  • Can we see feedback in action? Do we expect outflows enriching the intergalactic medium?

(Deadline: 9 July 2017)

Technische Universitaet Muenchen
Exzellenzcluster Universe

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D-85748 Garching

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