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.

Major new telescope on Chilean summit opens window on universe

Thirty-four years after Cornell University scientists first conceived it, the Fred Young Submillimeter Telescope (FYST) now rises above the Atacama Desert, near the summit of Cerro Chajnantor in Chile. FYST will help answer ...

Webb eyes a pair of planet-forming disks

This month's NASA/ESA/CSA James Webb Space Telescope Picture of the Month offers us a two-for-one on brand new stars—with some potential planets thrown in as well. This visual highlights Webb's views of the protoplanetary ...

Webb reveals hidden details of W51 star formation

A team of University of Florida researchers used the James Webb Space Telescope to capture photos of a star-forming region known as W51 with never-before-seen clarity and resolution. The long wavelengths of JWST's infrared ...

ALMA reveals teenage years of new worlds

Astronomers have, for the first time, captured a detailed snapshot of planetary systems in an era long shrouded in mystery. The ALMA survey to Resolve exoKuiper belt Substructures (ARKS), using the Atacama Large Millimeter/submillimeter ...

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