Juvela, MikaGuillet, VincentLiu, TieRistorcelli, IsabellePelkonen, Veli-MattiAlina, DanaBronfman, LeonardoEden, David J.Kim, Kee TaeKoch, Patrick M.Kwon, WoojinLee, Chang WonMalinen, JohannaMicelotta, ElisabettaMontillaud, JulienRawlings, Mark G.Sanhueza, PatricioSoam, ArchanaTraficante, AlessioYsard, NathalieZhang, Chuan-Peng2020-03-312020-03-312018-11-23Mika Juvela, Vincent Guillet, Tie Liu (2018) Dust spectrum and polarisation at 850 µm in the massive IRDC G035.39-00.33. Astronomy & Astrophysics.http://nur.nu.edu.kz/handle/123456789/4574Context. The sub-millimetre polarisation of dust emission from star-forming clouds carries information on grain properties and on the effects that magnetic fields have on cloud evolution. Aims. Using observations of a dense filamentary cloud G035.39-00.33, we aim to characterise the dust emission properties and the variations of the polarisation fraction.enAttribution-NonCommercial-ShareAlike 3.0 United Statessubmillimeterstars: protostarsArticle