Sofia/forcast observations of warm dust in S106: A fragmented environment

@article{Adams2015SofiaforcastOO,
  title={Sofia/forcast observations of warm dust in S106: A fragmented environment},
  author={J. Adams and T. Herter and J. Hora and N. Schneider and R. Lau and J. G. Staughn and R. Simon and N. Smith and R. Gehrz and L. Allen and S. Bontemps and S. Carey and G. Fazio and R. Gutermuth and A. G. Fernandez and M. Hankins and T. Hill and E. Keto and X. Koenig and K. Kraemer and S. Megeath and D. Mizuno and F. Motte and P. Myers and H. Smith},
  journal={The Astrophysical Journal},
  year={2015},
  volume={814},
  pages={54}
}
  • J. Adams, T. Herter, +22 authors H. Smith
  • Published 2015
  • Physics
  • The Astrophysical Journal
  • We present mid-IR (19–37 μm) imaging observations of S106 from SOFIA/FORCAST, complemented with IR observations from Spitzer/IRAC (3.6–8.0 μm), IRTF/MIRLIN (11.3 and 12.5 μm), and Herschel/PACS (70 and 160 μm). We use these observations, observations in the literature, and radiation transfer modeling to study the heating and composition of the warm (~100 K) dust in the region. The dust is heated radiatively by the source S106 IR, with little contributions from grain–electron collisions and Ly… CONTINUE READING
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