14 March 2016 | Gravitational torques imply molecular gas inflow towards the nucleus of M 51
| Querejeta, M; Meidt, SE; Schinnerer, E; et al. |
6 August 2020 | How do different spiral arm models impact the ISM and GMC population?
| Pettitt, AR; Dobbs, CL; Baba, J; et al. |
20 March 2014 | The PdBI Arcsecond Whirlpool Survey (PAWS): Environmental dependence of giant molecular cloud properties in M51
| Colombo, D; Hughes, A; Schinnerer, E; et al. |
20 March 2014 | The PdBI Arcsecond Whirlpool Survey (PAWS): Multi-phase cold gas kinematic of M51
| Colombo, D; Meidt, SE; Schinnerer, E; et al. |
8 February 2017 | The PdBI Arcsecond Whirlpool Survey (PAWS): The Role of Spiral Arms in Cloud and Star Formation
| Schinnerer, E; Meidt, SE; Colombo, D; et al. |
29 September 2021 | Perseus arm – a new perspective on star formation and spiral structure in our home galaxy
| Wienen, M; Brunt, CM; Dobbs, CL; et al. |
11 September 2020 | The SEDIGISM survey: First Data Release and overview of the Galactic structure
| Schuller, F; Urquhart, JS; Csengeri, T; et al. |
13 July 2022 | The SEDIGISM survey: Molecular cloud morphology. I. Classification and star formation
| Neralwar, KR; Colombo, D; Duarte-Cabral, A; et al. |
10 August 2022 | The SEDIGISM survey: Molecular cloud morphology. II. Integrated source properties
| Neralwar, KR; Colombo, D; Duarte-Cabral, A; et al. |
11 September 2020 | The SEDIGISM survey: Molecular clouds in the inner Galaxy
| Duarte-Cabral, A; Colombo, D; Urquhart, JS; et al. |
9 June 2015 | Short GMC lifetimes: an observational estimate with the PdBI Arcsecond Whirlpool Survey (PAWS)
| Meidt, SE; Hughes, A; Dobbs, CL; et al. |
19 December 2018 | The spatial relation between young star clusters and molecular clouds in M51 with LEGUS
| Grasha, K; Calzetti, D; Adamo, A; et al. |