Page 3: Research news on Submillimeter astronomy

Submillimeter astronomy is a research area focused on observing electromagnetic radiation at wavelengths between the far-infrared and millimeter regimes (roughly 0.1–1 mm), where cold dust, molecular gas, and cosmic microwave background–related processes emit strongly. It probes physical conditions in dense interstellar clouds, star-forming regions, circumstellar disks, and high-redshift galaxies via rotational transitions of molecules (e.g., CO) and thermal dust emission. The field relies on high-sensitivity, high-angular-resolution instruments such as bolometer arrays and heterodyne receivers, typically deployed on high, dry sites or space platforms to mitigate atmospheric water vapor absorption.

New method traces molecular gas mass in distant galaxies

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 ...

ALMA observes dusty site of planet formation

The Atacama Large Millimeter/submillimeter Array (ALMA) has successfully observed a site of planet formation by detecting a high concentration of dust grains, a planet-forming material, outside the orbits of just-formed planets.

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