Nearby Dusty Starbursts

摘要: Virtually all young starbursts are dusty, and hence can be understood only with a suite of techniques not strongly affected by extinction. Synthesis modeling developed around such provides satisfactory fits to the relevant observables. These models show that short-lived have extremely high star forming efficiency. Further advances will require improvements in way boundary conditions as bolometric K-band luminosity, ionizing effective temperature, supernova rate estimated applied models.