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Observations of high-order multiplicity in a high-mass stellar protocluster - Nature Astronomy

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Observations of high-order multiplicity in a high-mass stellar protocluster - Nature Astronomy

The dominant mechanism forming multiple stellar systems in the high-mass regime (M* ≳ 8 M⊙) remained unknown because direct imaging of multiple protostellar systems at early phases of high-mass star formation is very challenging. High-mass stars are expected to form in clustered environments containing binaries and higher-order multiplicity systems. So far only a few high-mass protobinary systems, and no definitive higher-order multiples, have been detected.

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Observations of high-order multiplicity in a high-mass stellar protocluster - Nature Astronomy

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Observations of high-order multiplicity in a high-mass stellar protocluster - Nature Astronomy

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