The high-velocity cloud G0.02 near the Galactic Center is better explained as gas on an eccentric orbit around the central mass than as a supernova remnant, based on new ALMA observations.
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Circum-nuclear eccentric gas flow in the Galactic Center revealed by ALMA CMZ Exploration Survey (ACES)
The high-velocity cloud G0.02 near the Galactic Center is better explained as gas on an eccentric orbit around the central mass than as a supernova remnant, based on new ALMA observations.