Far-infrared and molecular line observations of Lynds 183 - Studies of cold gas and dust

@article{Juvela2002FarinfraredAM,
  title={Far-infrared and molecular line observations of Lynds 183 - Studies of cold gas and dust},
  author={M. Juvela and K. Mattila and K. Lehtinen and D. Lemke and R. Laureijs and T. Prusti},
  journal={Astronomy and Astrophysics},
  year={2002},
  volume={382},
  pages={583-599}
}
We have mapped the dark cloud L183 in the far-infrared at 100 m and 200 m with the ISOPHOT photometer aboard the ISO satellite. The observations make it possible for the rst time to study the distribution and properties of the large dust grains in L183 without confusion from smaller grains. The observations show clear colour temperature variations which are likely to be caused by changes in the emission properties of the dust particles. In the cloud core the far-infrared colour temperature… Expand
Direct evidence of dust growth in L183 from MIR light scattering
FUSE observations of molecular hydrogen on the line of sight towards HD 141569A
Far infrared observations of pre-protostellar sources in Lynds 183
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