New observations have confirmed a key step in the process of star formation: a rotating “cosmic wind” made of molecules, which is vitally important for collapsing gas clouds to contract sufficiently so as to form a hot, dense young star. The result was obtained from radio observations, combined with a sophisticated analysis that allowed astronomers to probe the flow of matter around a young star in the dark cloud CB26 in greater detail than ever before. The work has been published in the journal Astronomy & Astrophysics.
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