The role of protostellar jets in star formation and the evolution of the early solar system: Astrophysical and meteoritical perspectives
作者： Raquel SALMERON , Trevor IRELAND
DOI: 10.1111/MAPS.12029
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摘要: – The rock record from the early solar system indicates high-temperature thermal processing sufficient to melt refractory oxides and silicates. astrophysical context for formation evolution of our system, a molecular cloud “clean” planetary is difficult constrain tightly because large scales lack resolution astronomical observations. Protostellar jets winds, commonly associated with forming stars, are likely play role in heating redistribution processed material system. We have recently proposed that disk-winds can cause melting small inclusions distances out several AU. Particularly energetic outbursts, such as FU-Orionis EXor events, occur over relatively short time (approximately 100 1 yr, respectively), probably events related solids present primitive meteorites.
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