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Paper: A Multi-Species Multi-Wavelength View of the Sgr A Complex
Volume: 528, New Horizons in Galactic Center Astronomy and Beyond
Page: 309
Authors: García, P.; Steinke, M.; Simon, R; Stutzki, J.
Abstract: Here we present the current status of our ongoing multi-species (12CO, 13CO, C18O, C17O, HCO+, H13CO+, HCN, and H13CN) multi-wavelength (rotational numbers Jupper = 4, 3, 2, 1, and hyperfine splitting) observations targeting ten positions at the Sgr A Complex tracing the spatial distribution of the major gas agglomerates detected in CO(4-3) observations of this region (García et al. 2016). In combination with the C+, C, and 12CO sub-millimeter observations in García et al. (2016), a total of ∼26 transitions are detected at all positions. These rich data sets will allow us to study in detail the physical conditions of the gas and their large-scale spatial trends across the Sgr A Complex, yielding a comprehensive view of the ISM within the GC.
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