TY  -  
T1  - Dust spectrum and polarisation at 850 mu m in the massive IRDC G035.39-00.33 
SN  -  /  
UR  - http://hdl.handle.net/10138/307874 
T3  -  
A1  - Juvela, Mika; Guillet, Vincent; Liu, Tie; Ristorcelli, Isabelle; Pelkonen, Veli-Matti; Alina, Dana; Bronfman, Leonardo; Eden, David J.; Kim, Kee Tae; Koch, Patrick M.; Kwon, Woojin; Lee, Chang Won; Malinen, Johanna; Micelotta, Elisabetta; Montillaud, Julien; Rawlings, Mark G.; Sanhueza, Patricio; Soam, Archana; Traficante, Alessio; Ysard, Nathalie; Zhang, Chuan-Peng 
A2  -  
PB  -  
Y1  - 2018 
LA  - eng 
AB  - Context. 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. Methods. JCMT SCUBA-2/POL-2 observations at 850 mu m were combined with Planck 850 mu m (353 GHz) data to map polarisation fraction at small a... 
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KW  - ISM: clouds; infrared: ISM; submillimeter: ISM; dust, extinction; stars: formation; stars: protostars; GOULD BELT SURVEY; MAGNETIC-FIELD; GRAIN ALIGNMENT; MOLECULAR CLOUD; DARK CLOUD; RADIATIVE TORQUES; INFRARED OBSERVATIONS; SCUBA-2 OBSERVATIONS; TAURUS; POLARIMETRY; 115 Astronomy, Space science 
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