  Star-forming regions are often associated with nebulosity. In this study, we
investigated infrared diffuse emission in Spitzer IRAC images. The infrared
nebula L1527 traces outflows emanating from a low-mass protostar. The nebular
color is consistent with the color of a stellar photosphere with large
extinction. Nebulae around the HII region W5-East are bright in the infrared.
These colors are consistent with the model color of dust containing polycyclic
aromatic hydrocarbon (PAH). The strength of ultraviolet irradiation of the
nebulae and the small dust fraction were deduced from the infrared colors of
the nebulae. We found that the edges of the nebulae are irradiated by strong
ultraviolet radiation and have abundant small dust. Dust at the surface of the
molecular cloud is thought to be destroyed by ultraviolet radiation from an
early-type star.
