ListarArtículos científicos por tema "Techniques: interferometric"
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Fragmentation in the massive G31.41+0.31 protocluster (2021)
(EDP Sciences, 2021-04-01)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 ... -
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Kinematics and stability of high-mass protostellar disk candidates at sub-arcsecond resolution: Insights from the IRAM NOEMA large programme CORE (2024)
(EDP Sciences, 2023)Context. The fragmentation mode of high-mass molecular clumps and the accretion processes that form the most massive stars (M ≳ 8 M·) are still not well understood. A growing number of case studies have found massive young ... -
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Multi-scale view of star formation in IRAS 21078+5211: From clump fragmentation to disk wind (2021)
(EDP Sciences, 2021-03-01)Context. Star formation (SF) is a multi-scale process in which the mode of fragmentation of the collapsing clump on scales of 0.1-1 pc determines the mass reservoir and affects the accretion process of the individual ...