MODEL INFRARED SPECTRA FOR PROTO STARS

  • Published : 1997.12.01

Abstract

We have modeled the infrared spectral energy distributions of proto stars with close attention to the dust envelopes around the stars. The observed spectral energy distributions are closely compared with our models. The model results and observations are compared on IRAS color-color diagrams. Typical model results can explain the observations fairly well.

Keywords

References

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