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Published online by Cambridge University Press: 26 May 2016
An overview of some key results related to hot, massive stars and starbursts in the infrared is given. The wavelength range covers the ground- and space-based near-infrared, the mid- and far-IR as probed by several space missions, and the sub-millimeter regime. I discuss how these observations permit an unbiased view of dust-obscured stars and how they are related to data at optical and ultraviolet wavelengths.