Disk masses in the Orion Molecular Cloud-2

The mass evolution of protoplanetary disks is driven by internal processes and by external factors such as photoevaporation. Disentangling these two effects, however, remains...原行星盘（protoplanetary disks）的质量演化由内部过程与光致蒸发（photoevaporation）等外部因素共同驱动。然而，厘清这两类效应的相对贡献仍有待进一步研究。