Radio background and IGM heating due to Pop III supernova explosions

Author:

Jana Ranita1ORCID,Nath Biman B1,Biermann Peter L23

Affiliation:

1. Raman Research Institute, Sadashiva Nagar, Bangalore 560080, India

2. Max Planck Institut für Radioastronomie, Auf dem Hügel 69, Bonn, Germany

3. Department of Physics, Karlsruhe Institut für Technologie, Karlsruhe, Germany

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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