Linked from

The 8 pages that link to Photoevaporation, each with the reason it gives.

• Protoplanetary diskRelated: Radiation from the star and its surroundings helps disperse disk gas.

• Eagle NebulaRelated: Ultraviolet radiation erodes exposed gas at the pillars’ surfaces.

• Bok globuleRelated: Ultraviolet light can remove a globule's outer gas before collapse is complete.

• Pillars of CreationRelated: Radiation from nearby massive stars erodes the pillars’ exposed surfaces.

• ProplydRelated: Ultraviolet heating drives gas off the disk and forms its outward-flowing envelope.

• Trapezium ClusterRelated: Ultraviolet light from massive cluster stars strips gas from nearby protoplanetary disks.