It is probable that primordial galaxies triggered the period in the history of the universe known as "cosmic reionization." The Geneva-based astronomer Anne Verhamme has succeeded in demonstrating this by studying green pea galaxies. In recognition of this work, the SNSF will award her this year's Marie Heim-Vogtlin prize on 16 September 2019.
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This Hubble image shows the green pea galaxy J0925+1403 [Credit: NASA] |
These stars must have emitted large quantities of ultraviolet radiation that was capable of ionizing the hydrogen atoms, because astronomers observed that electrons and protons separated again a billion years after the Big Bang. This is what we call the cosmic reionization period.
Successful new measurement technique
For a long time, astronomers could not explain where the powerful UV radiation needed for reionization had come from. The majority of observed galaxies do not emit ionizing photons and the few known exceptions emit too little to keep the universe ionized.
Anne Verhamme, professor of astronomy at the University of Geneva, proposed that green pea galaxies—a new type of galaxy discovered ten years ago—probably emit large quantities of ionizing photons.
This assumption was based on the highly specific properties of rays emitted by the hydrogen atoms in these galaxies, known as Lyman-alpha radiation. Astronomers believe that green pea galaxies resemble primordial galaxies as they are extremely compact, are creating their first generations of stars, and are still rich in gas.
Using data from the Hubble Space Telescope, Anne Verhamme and a international team of collaborators were able to demonstrate that green pea galaxies do indeed emit large quantities of ionizing photons. If green peas are analogous to primordial galaxies, it seems very likely that it was galaxies that triggered the reionization of the universe more than 13 billion years ago.
The papers were published in Astronomy & Astrophysics in 2015 & 2016.
Source: Swiss National Science Foundation [August 28, 2019]
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