[C II] 158 Micron Emission and CO(1-0) Line
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alternative H2 tracersPhys Org
•New method traces molecular gas mass in distant galaxies
91% Informative
The traditional tracer for H2 mass, the CO(1-0) line, is challenging to detect in the early universe due to various factors, including lower metal content.
In recent years , the [C II] 158 micron emission has emerged as a promising tool for investigating the gas content in the distant universe.
Their findings were published in The Astrophysical Journal .
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