Millimeter wave spectral line surveys and line mapping studies of NGC6334I and I(N)

S. Thorwirth; A. J. Walsh; F. Wyrowski; P. Schilke; H. Beuther; T. R. Hunter; C. Comito; S. Leurini; A. R. Tieftrunk; M. G. Burton; K. M. Menten

arXiv · 0709.3776

Millimeter wave spectral line surveys and line mapping studies of NGC6334I and I(N)

S. Thorwirth·A. J. Walsh·F. Wyrowski·P. Schilke·H. Beuther·T. R. Hunter·C. Comito·S. Leurini·A. R. Tieftrunk·M. G. Burton·K. M. Menten

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Abstract

NGC6334I and I(N) have been observed with the Swedish-ESO Submillimetre Telescope, SEST, at wavelengths of 3, 2, and 1.3 mm. Especially NGC6334 I shows rich emission from many different molecules, comparable in line density to prototypical hot cores such as Orion-KL and SgrB2(N). In addition, a 4' by 4' region enfolding NGC 6334 I and I(N) has been mapped at a wavelength of 3 mm (75 to 116 GHz) with the Mopra telescope.

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S. Thorwirth, A. J. Walsh, F. Wyrowski, P. Schilke, H. Beuther, T. R. Hunter, C. Comito, S. Leurini, A. R. Tieftrunk, M. G. Burton, K. M. Menten. 2007-09-24. Millimeter wave spectral line surveys and line mapping studies of NGC6334I and I(N). https://arxiv.org/abs/0709.3776

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