气体纤维状结构与纤维间结构如何为麒麟座 R2 的恒星形成提供物质

研究人员通过追踪一氧化碳的流动，分析了麒麟座 R2 产星区内气体向恒星形成中心汇聚的过程。研究发现，纤维状结构与纤维间结构共同构成了物质输送系统，为恒星形成区域提供气体补给。

Researchers studied gas flows in the Monoceros R2 star forming region to understand how gas is channeled into star forming hubs. By tracing the flow of carbon monoxide, they found that a system of hub-filaments and interfilaments are responsible for feeding gas into star-forming locations. The filaments move most of the gas, but the interfilaments play a role too, especially by feeding more gas into the main filaments.