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

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

2007-09-24

arxiv.org/abs/0709.3776v1

Astronomy and Astrophysics

Astrophysics

2 pages, 2 figures, to appear in Conference Proceedings "Molecules in Space and Laboratory"

Scientific paper

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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