Astronomers Develop New Models to Search for Molecular Oxygen

Newly published research from the Harvard-Smithsonian Center for Astrophysics provides the first self-consistent treatment of preshock, shock, and postshock regions under the influence of UV fields, and explains why O2 detections are so rare. Oxygen is the third most abundant element in the universe (after hydrogen and helium) and of course it is important: all […]
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