Abstract.
We report on mid-infrared imaging of hot cores performed with SpectroCam-10 and TIMMI2. The observations aimed at the detection of thermal emission presumably associated with the hot cores. Mid-infrared flux measurements are required to improve the luminosity and optical depth estimates for these sources. Results are presented for W3(H2O), G9.62+0.19, G10.47+0.03, and the possible hot core candidate G232.620+0.996. They illustrate that the morphology of these sources cannot be described by simple geometries. Therefore, line-of-sight effects and considerable extinction even at mid-infrared wavelengths must not be neglected.
Based on observations collected at the European Southern Observatory, La Silla, Chile, Proposal IDs 62.I-0530,67.C-0359
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Stecklum, B., Brandl, B., Feldt, M., Henning, T., Linz, H., Pascucci, I. Infrared Observation of Hot Cores. In: Alves, J.F., McCaughrean, M.J. (eds) The Origin of Stars and Planets: The VLT View. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10856518_28
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DOI: https://doi.org/10.1007/10856518_28
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