A multi-wavelength observation and investigation of six infrared dark clouds
arXiv:1611.08794 · doi:10.1051/0004-6361/201629771
Abstract
Context. Infrared dark clouds (IRDCs) are ubiquitous in the Milky Way, yet they play a crucial role in breeding newly-formed stars. Aims. With the aim of further understanding the dynamics, chemistry, and evolution of IRDCs, we carried out multi-wavelength observations on a small sample. Methods. We performed new observations with the IRAM 30 m and CSO 10.4 m telescopes, with tracers , HCN, , , DCO, SiO, and DCN toward six IRDCs G031.97+00.07, G033.69-00.01, G034.43+00.24, G035.39-00.33, G038.95-00.47, and G053.11+00.05. Results. We investigated 44 cores including 37 cores reported in previous work and seven newly-identified cores. Toward the dense cores, we detected 6 DCO, and 5 DCN lines. Using pixel-by-pixel spectral energy distribution (SED) fits of the 70 to 500 m, we obtained dust temperature and column density distributions of the IRDCs. We found that emission has a strong correlation with the dust temperature and column density distributions, while showed the weakest correlation. It is suggested that is indeed a good tracer in very dense conditions, but is an unreliable one, as it has a relatively low critical density and is vulnerable to freezing-out onto the surface of cold dust grains. The dynamics within IRDCs are active, with infall, outflow, and collapse; the spectra are abundant especially in deuterium species. Conclusions. We observe many blueshifted and redshifted profiles, respectively, with and toward the same core. This case can be well explained by model "envelope expansion with core collapse (EECC)".
arXiv comment24 pages, 11 figures, 4 tables. To be published in A&A. The resolutions of the pictures are cut down
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