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From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt Survey
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Characterizing interstellar filaments with Herschel in IC 5146
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Physical properties of interstellar filaments
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Cores, filaments, and bundles: hierarchical core formation in the L1495/B213 Taurus region
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Herschel view of the Taurus B211/3 filament and striations: evidence of filamentary growth?
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Planck 2013 results. XI. All-sky model of thermal dust emission
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A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey
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November 2015 |
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Planck intermediate results : XXXV. Probing the role of the magnetic field in the formation of structure in molecular clouds
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Filamentary structure and magnetic field orientation in Musca
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May 2016 |
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The relation between the column density structures and the magnetic field orientation in the Vela C molecular complex
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July 2017 |
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Characterizing the properties of nearby molecular filaments observed with Herschel
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January 2019 |
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ALMA reveals the magnetic field evolution in the high-mass star forming complex G9.62+0.19
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June 2019 |
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Probing accretion of ambient cloud material into the Taurus B211/B213 filament
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February 2019 |
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The role of molecular filaments in the origin of the prestellar core mass function and stellar initial mass function
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August 2019 |
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High-accuracy estimation of magnetic field strength in the interstellar medium from dust polarization
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Why take the square root? An assessment of interstellar magnetic field strength estimation methods
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The Equilibrium of Polytropic and Isothermal Cylinders.
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The linear polarization of quasi-stellar radio sources at 3.71 and 11.1 centimeters
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A study of the Taurus dark cloud complex
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September 1978 |
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December 1988 |
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Photoionization-regulated star formation and the structure of molecular clouds
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Magnetic field-line tangling and polarization measurements in clumpy molecular gas
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On the dispersion in direction of interstellar polarization
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May 1991 |
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Equiparatition of energy for turbulent astrophysical fluids: Accounting for the unseen energy in molecular clouds
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9286 Stars: an Agglomeration of Stellar Polarization Catalogs
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February 2000 |
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A Production Mechanism for Clusters of Dense Cores
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Weakly Compressible Magnetohydrodynamic Turbulence in the Solar Wind and the Interstellar Medium
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The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-gravitational Hydrodynamics
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Density, Velocity, and Magnetic Field Structure in Turbulent Molecular Cloud Models
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January 2001 |
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Theoretical Models of Polarized Dust Emission from Protostellar Cores
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October 2001 |
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Magnetic Field Diagnostics Based on Far‐Infrared Polarimetry: Tests Using Numerical Simulations
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November 2001 |
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Studies of Regular and Random Magnetic Fields in the ISM: Statistics of Polarization Vectors and the Chandrasekhar‐Fermi Technique
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May 2008 |
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Magnetically Aligned Velocity Anisotropy in the Taurus Molecular Cloud
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June 2008 |
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Dispersion of Magnetic Fields in Molecular Clouds. i
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Dispersion of Magnetic Fields in Molecular Clouds. ii.
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Magnetic Fields in Interstellar Clouds from Zeeman Observations: Inference of Total Field Strengths by Bayesian Analysis
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November 2010 |
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Magnetic Field Structure Around Low-Mass Class 0 Protostars: B335, L1527, and Ic348-Smm2
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April 2011 |
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The Magnetic Field in Taurus Probed by Infrared Polarization
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October 2011 |
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A Stable, Accurate Methodology for high mach Number, Strong Magnetic Field mhd Turbulence with Adaptive mesh Refinement: Resolution and Refinement Studies
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Is the Taurus b213 Region a true Filament?: Observations of Multiple Cyanoacetylene Transitions
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August 2012 |
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The Fragmentation of Magnetized, Massive Star-Forming Cores with Radiative Feedback
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March 2013 |
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An Imprint of Molecular Cloud Magnetization in the Morphology of the dust Polarized Emission
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August 2013 |
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Magnetohydrostatic Equilibrium Structure and mass of Filamentary Isothermal Cloud Threaded by Lateral Magnetic Field
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March 2014 |
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From parallel to perpendicular – On the orientation of magnetic fields in molecular clouds
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August 2020 |
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Gravitational instability of non-isothermal filamentary molecular clouds in presence of external pressure
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February 2021 |
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Magnetized interstellar molecular clouds – I. Comparison between simulations and Zeeman observations
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July 2015 |
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A census of dense cores in the Taurus L1495 cloud from the Herschel Gould Belt Survey
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February 2016 |
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Magnetized interstellar molecular clouds – II. The large-scale structure and dynamics of filamentary molecular clouds
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March 2019 |
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Near-infrared imaging polarimetry toward M 17 SWex
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July 2019 |
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The Strength of Interstellar Magnetic Fields
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March 1951 |
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CRUSH: fast and scalable data reduction for imaging arrays
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August 2008 |
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HAWC+, the Far-Infrared Camera and Polarimeter for SOFIA
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December 2018 |
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Gravitational Instability of the Isothermal Gas Cylinder with an Axial magnetic Field
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March 1987 |
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Theory of Star Formation
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Cold Dark Clouds: The Initial Conditions for Star Formation
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Dispersion of Magnetic Fields in Molecular Clouds. iv. Analysis of Interferometry data
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March 2016 |
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Change of Magnetic Field-Gas Alignment at the Gravity-Driven AlfvÉNic Transition in Molecular Clouds: Implications for dust Polarization Observations
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September 2016 |
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Morphology and Kinematics of Filaments in the Serpens and Perseus Molecular Clouds
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February 2018 |
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The Emission and Distribution of Dust of the Torus of NGC 1068
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May 2018 |
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JCMT POL-2 and BISTRO Survey Observations of Magnetic Fields in the L1689 Molecular Cloud
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February 2021 |
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Maps of Magnetic Field Strength in the OMC-1 Using HAWC+ FIR Polarimetric Data
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February 2021 |
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Magnetohydrostatic Equilibrium Structure and Mass of Polytropic Filamentary Cloud Threaded by Lateral Magnetic Field
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April 2021 |
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Magnetic Properties of Star-forming Dense Cores
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August 2021 |
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The JCMT BISTRO Survey: Revealing the Diverse Magnetic Field Morphologies in Taurus Dense Cores with Sensitive Submillimeter Polarimetry
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May 2021 |