GASS 3505: A Hydrogen Rich, Passive Galaxy

New research from the Harvard-Smithsonian Center for Astrophysics reveals that the star formation in GASS 3505 is very weak, less than about 0.1 solar-masses per year. Cold gas in the form of neutral hydrogen atoms provides the reservoir for star formation in galaxies from the distant to the nearby Universe. Understanding how it accretes onto […]
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