Prof. Zhao Yinghe from the Yunnan Observatories of the Chinese Academy of Sciences, along with collaborators, have conducted a study examining the correlation between the [C II] 158 micron emission and the CO(1−0) line. Their findings were published in The Astrophysical Journal.
Molecular gas (H2) plays a critical role in star formation, a key factor in the evolution of galaxies. Therefore, measuring the gas content in galaxies is crucial. However, 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.
As a result, there is a pressing need for alternative H2 tracers, especially as more galaxies at high redshifts are being discovered.