A recent study led by researchers at the Max Planck Institute for Extraterrestrial Physics challenges conventional notions of star formation by revealing the intricate connection between streamers and filaments. Focusing on the star-forming region Barnard 5, the study traces the journey of material from larger scales to protostellar disks, uncovering a remarkable relationship between elongated filaments and gas streamers. In particular, the team discovered a sizeable streamer, which suggests that young stars can receive additional material even after the so-believed main accretion phase.
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