The new observations using ALMA’s Band 6 (1.3mm wavelength) receiver— developed by the U.S. National Science Foundation‘s National Radio Astronomy Observatory (NRAO)— allowed scientists to zoom into three key regions in extreme detail, and for the first time, build a clear picture of how the hydrogen gas is moving and being shaped on a continuous basis.
“The power of ALMA is obvious in these observations, providing astronomers new insights and better understanding of these previously unknown processes,” said Joe Pesce, Program Officer for ALMA at the U.S. National Science Foundation (NSF).
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