SEDIGISM-ATLASGAL: dense gas fraction and star formation efficiency across the Galactic disc

J Urquhart , C Figura , J. Cross (1) , M Wells , T. Moore (2) , D Eden , S Ragan , A. Pettitt (3) , A. Duarte-Cabral (4) , D. Colombo , F Schuller , T Csengeri (5) , M Mattern (6) , H Beuther , K Menten , F Wyrowski , L Anderson , P Barnes , M Beltrán , S Billington , L Bronfman , A Giannetti , J Kainulainen , J Kauffmann , M-y Lee , S Leurini , S-N Medina , F Montenegro-Montes , M Riener , A Rigby , A Sánchez-Monge , P Schilke , E Schisano , A Traficante , M Wienen

1 Department of Physics [Oxford]
2 GSFC - NASA Goddard Space Flight Center
3 Oxford National Institute for Health Research Biomedical Research Centre/Molecular Diagnostic Centre
4 School of Physics and Astronomy [Cardiff]
5 FORMATION STELLAIRE 2020
6 AIM (UMR_7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation

Domaines: Astrophysique [astro-ph]

J Urquhart, C Figura, J. Cross, M Wells, T. Moore, et al.. SEDIGISM-ATLASGAL: dense gas fraction and star formation efficiency across the Galactic disc. Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3050-3063. ⟨10.1093/mnras/staa2512⟩. ⟨hal-03046484⟩