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Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/188959
Fragmentation and cluster formation in the Infrared Dark Cloud G14.225−0.506
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We obtained images of the G14.2 Hub-S with data acquired by ALMA. The visibilities were weighted naturally and with robust=0 with the task tclean of CASA to get different spatial resolutions (160 and 64 AU, respectively). We identified 22 sources with the tool PyBDSF and we estimated their masses and sizes. We found that most of the sources correspond to low-mass protostellar disks but there is a large mass reservoir in the envelope that can feed the protostar to become high-mass stars
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Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutora: Gemma Busquet Rico
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TORRES DURAN, Eduard. Fragmentation and cluster formation in the Infrared Dark Cloud G14.225−0.506. [consulted: 18 of June of 2026]. Available at: https://hdl.handle.net/2445/188959