Observations of Snake III demonstrate that molecular cloud density and early feedback jointly regulate the sequence of star formation, with older clusters in cavities and young stars forming in dense regions.
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The Stellar "Snake"-III: Co-evolution of Stars and Molecular Clouds Unveiled by Gaia, MWISP, and LAMOST
Observations of Snake III demonstrate that molecular cloud density and early feedback jointly regulate the sequence of star formation, with older clusters in cavities and young stars forming in dense regions.