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BALLOON-BORNE SUBMILLIMETER POLARIMETRY OF THE VELA C MOLECULAR CLOUD: SYSTEMATIC DEPENDENCE OF POLARIZATION FRACTION ON COLUMN DENSITY AND LOCAL POLARIZATION-ANGLE DISPERSION
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Matching dust emission structures and magnetic field in high-latitude cloud L1642: comparingHerschelandPlanckmaps
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The magnetic field and dust filaments in the Polaris Flare
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Probing interstellar turbulence in cirrus with deep optical imaging: no sign of energy dissipation at 0.01 pc scale
Galactic interstellar filaments as probed by LOFAR and Planck
S. Zaroubi, V. Jelić, A. G. de Bruyn, F. Boulanger, A. Bracco, R. Kooistra, M. I. R. Alves, M. A. Brentjens, K. Ferrière, T. Ghosh, L. V. E. Koopmans, F. Levrier, M.-A. Miville-Deschênes, L. Montier, V. N. Pandey and J. D. Soler Monthly Notices of the Royal Astronomical Society: Letters 454(1) L46 (2015) https://doi.org/10.1093/mnrasl/slv123
Searching for inflationary B modes: can dust emission properties be extrapolated from 350 GHz to 150 GHz?
Konstantinos Tassis and Vasiliki Pavlidou Monthly Notices of the Royal Astronomical Society: Letters 451(1) L90 (2015) https://doi.org/10.1093/mnrasl/slv077
Planckintermediate results. XIX. An overview of the polarized thermal emission from Galactic dust