Dust spectrum and polarisation at 850 µm in the massive IRDC G035.39-00.33

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dc.contributor.authorJuvela, Mika
dc.contributor.authorGuillet, Vincent
dc.contributor.authorLiu, Tie
dc.contributor.authorRistorcelli, Isabelle
dc.contributor.authorPelkonen, Veli-Matti
dc.contributor.authorAlina, Dana
dc.contributor.authorBronfman, Leonardo
dc.contributor.authorEden, David J.
dc.contributor.authorKim, Kee Tae
dc.contributor.authorKoch, Patrick M.
dc.contributor.authorKwon, Woojin
dc.contributor.authorLee, Chang Won
dc.contributor.authorMalinen, Johanna
dc.contributor.authorMicelotta, Elisabetta
dc.contributor.authorMontillaud, Julien
dc.contributor.authorRawlings, Mark G.
dc.contributor.authorSanhueza, Patricio
dc.contributor.authorSoam, Archana
dc.contributor.authorTraficante, Alessio
dc.contributor.authorYsard, Nathalie
dc.contributor.authorZhang, Chuan-Peng
dc.date.accessioned2020-03-31T09:40:23Z
dc.date.available2020-03-31T09:40:23Z
dc.date.issued2018-11-23
dc.description.abstractContext. 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.en_US
dc.identifier.citationMika Juvela, Vincent Guillet, Tie Liu (2018) Dust spectrum and polarisation at 850 µm in the massive IRDC G035.39-00.33. Astronomy & Astrophysics.en_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/4574
dc.language.isoenen_US
dc.publisherAstronomy & Astrophysicsen_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectsubmillimeteren_US
dc.subjectstars: protostarsen_US
dc.titleDust spectrum and polarisation at 850 µm in the massive IRDC G035.39-00.33en_US
dc.typeArticleen_US
workflow.import.sourcescience

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