Now showing items 1-12 of 12

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