YSO candidates within 5' from the IR bubble N4
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https://b2find.eudat.eu/dataset/8edebdf9-98fb-5db1-a2dd-da7e8f43d7a9
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The physical mechanisms that induce the transformation of a certain mass of gas in new stars are far from being well understood. Infrared bubbles associated with H II regions...
驱动特定气团转化为新生恒星的物理机制，目前仍远未被完全阐明。与电离氢区（H II regions）相关联的红外气泡……
