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Get Free AccessContext. 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.
F. Schüller, T. Csengeri, J. S. Urquhart, A. Duarte-Cabral, Peter J Barnes, A. Giannetti, Audra K. Hernandez, S. Leurini, M. Mattern, S.-N. X. Medina, C. Agurto, F. Azagra, L. D. Anderson, M. T. Beltrán, H. Beuther, N. Schneider, L. Bronfman, Clare L. Dobbs, M. Dumke, Ricardo Finger, Adam Ginsburg, Elizabeth Johana Gonzalez, Thomas Henning, Jens Kauffmann, F. Mac-Auliffe, K. M. Menten, F. M. Montenegro‐Montes, T. J. T. Moore, Erik Muller, Rodrigo Parra, J. P. Pérez-Beaupuits, Alex R. Pettitt, D. Russeil, Á. Sánchez-Monge, P. Schilke, E. Schisano, S. Suri, L. Testi, K. Torstensson, Paulina Venegas, Ke Wang, M. Wienen, F. Wyrowski, A. Zavagno (2017). SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium. , 601, DOI: https://doi.org/10.1051/0004-6361/201628933.
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Type
Article
Year
2017
Authors
44
Datasets
0
Total Files
0
Language
en
DOI
https://doi.org/10.1051/0004-6361/201628933
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