SEDIGISM: Structure, excitation, and dynamics of the inner Galactic interstellar medium

Context. 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. Neverthele...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2017-05, Vol.601, p.A124
Hauptverfasser:	Schuller, F., Csengeri, T., Urquhart, J. S., Duarte-Cabral, A., Barnes, P. J., Giannetti, A., Hernandez, A. K., Leurini, S., Mattern, M., Medina, S.-N. X., Agurto, C., Azagra, F., Anderson, L. D., Beltrán, M. T., Beuther, H., Bontemps, S., Bronfman, L., Dobbs, C. L., Dumke, M., Finger, R., Ginsburg, A., Gonzalez, E., Henning, T., Kauffmann, J., Mac-Auliffe, F., Menten, K. M., Montenegro-Montes, F. M., Moore, T. J. T., Muller, E., Parra, R., Perez-Beaupuits, J.-P., Pettitt, A., Russeil, D., Sánchez-Monge, Á., Schilke, P., Schisano, E., Suri, S., Testi, L., Torstensson, K., Venegas, P., Wang, K., Wienen, M., Wyrowski, F., Zavagno, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Aerial surveys Angular resolution Astrophysics Clouds Clumps Data reduction Excitation Galactic Astrophysics Galactic evolution Galaxies Galaxy: structure Interstellar chemistry Interstellar matter ISM: clouds ISM: structure Molecular chains Molecular clouds Molecular gases Natural gas Optical analysis radio lines: ISM Rotation Sciences of the Universe surveys
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