HAL (France)
open access
Anatomy of the Class I protostar L1489 IRS with NOEMA. II. A disk replenished by a massive streamer
Context . Streamers are newly identified channels that transport mass from large, molecular-cloud scales down to small, protoplanetary-disk scales. To better understand their impact on planet formation, it is essential to study their physical and chemical properties. Aims . In this framework, we aim
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