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

Simple item page
dc.creatorThorwirth, S.
dc.creatorWalsh, A. J.
dc.creatorWyrowski, F.
dc.creatorSchilke, P.
dc.creatorBeuther, H.
dc.creatorHunter, T. R.
dc.creatorComito, C.
dc.creatorLeurini, S.
dc.creatorTieftrunk, A. R.
dc.creatorBurton, M. G.
dc.creatorMenten, K. M.
dc.date2007-09-24
dc.date.accessioned2026-07-07T08:31:50Z
dc.date.available2026-07-07T08:31:50Z
dc.descriptionNGC6334I 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.
dc.description2 pages, 2 figures, to appear in Conference Proceedings "Molecules in Space and Laboratory"
dc.identifierhttps://arxiv.org/abs/0709.3776
dc.identifierhttp://arxiv.org/abs/0709.3776
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/138617
dc.subjectAstrophysics
dc.titleMillimeter wave spectral line surveys and line mapping studies of NGC6334I and I(N)
dc.typetext

Files

Collections

arXiv