Schuller, F, Csengeri, T, Urquhart, JS, Duarte-Cabral, A, Barnes, PJ, Giannetti, A, Hernandez, AK, Leurini, S, Mattern, M, Medina, S-NX et al (show 34 more authors)
(2017)
SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium.
ASTRONOMY & ASTROPHYSICS, 601.
A124-A124.
Abstract
The origin and life-cycle of molecular clouds are still poorly constrained, despite their importance for understanding the evolution of the interstellar medium. Many large-scale surveys of the Galactic plane have been conducted recently, allowing for rapid progress in this field. Nevertheless, a sub-arcminute resolution global view of the large-scale distribution of molecular gas, from the diffuse medium to dense clouds and clumps, and of their relationshipto the spiral structure, is still missing. Aims. We have carried out a systematic, homogeneous, spectroscopic survey of the inner Galactic plane, in order to complement the many continuum Galactic surveys available with crucial distance and gas-kinematic information. Our aim is to combine this data set with recent infrared to sub-millimetre surveys at similar angular resolutions.
| Item Type: | Article |
|---|---|
| Uncontrolled Keywords: | surveys, Galaxy: structure, radio lines: ISM, ISM: clouds, ISM: structure |
| Depositing User: | Symplectic Admin |
| Date Deposited: | 16 Nov 2018 11:17 |
| Last Modified: | 19 Jan 2023 01:26 |
| DOI: | 10.1051/0004-6361/201628933 |
| Open Access URL: | https://arxiv.org/pdf/1701.04712.pdf |
| Related URLs: | |
| URI: | https://livrepository.liverpool.ac.uk/id/eprint/3025496 |
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