Repositorio de Universidad Autónoma de Chile.
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Fragmentation in the massive G31.41+0.31 protocluster
Context. ALMA observations at 1.4 mm and 0.′′2 (750 au) angular resolution of the Main core in the high-mass star-forming region G31.41+0.31 have revealed a puzzling scenario. On the one hand, the continuum emission looks very homogeneous and the core appears to undergo solid-body rotation, suggesti
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