Astronomers detect first direct evidence of star-forming gas in early galaxies
The first galaxies were already busy by the time the universe was 700 to 800 million years old. Stars were forming fast. Structures were taking shape. Additionally, huge stores of gas were feeding that growth. What astronomers have struggled to see clearly is the neutral gas at the center of that process. It is the cooler material that directly supplies star formation. That missing piece has now come into view. An international team led by Assistant Professor Yoshinobu Fudamoto and Professor Masamune Oguri of Chiba University used the Atacama Large Millimeter/submillimeter Array, or ALMA, to detect the [O I] 145 micrometer emission line in four distant galaxies. The signal comes from neutral oxygen and serves as a direct tracer of neutral gas. As a result, it is a powerful way to study the material that fuels early star formation. The galaxies were seen as they existed more than 13 billion years ago, at redshifts above 6.5. According to the team, this is the most distant direct detection yet of neutral gas in typical star-forming galaxies. …







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