Formation of free-floating planetary mass objects via circumstellar disk encounters
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DOI: 10.1126/sciadv.adu6058
Abstract: The origin of planetary mass objects (PMOs) wandering in young star clusters remains enigmatic, especially when they come in pairs. They could represent the lowest-mass object formed via molecular cloud collapse or high-mass planets ejected… read more here.
Keywords: formation free; mass; mass objects; floating planetary ... See more keywords