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Imaging polarimetry of class I young stellar objects
P.W. Lucas
, P.F. Roche
Centre for Astrophysics Research (CAR)
School of Physics, Engineering & Computer Science
Department of Physics, Astronomy and Mathematics
Centre for Future Societies Research
Research output
:
Contribution to journal
›
Article
›
peer-review
47
Citations (Scopus)
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Keyphrases
Young Stellar Objects
100%
Imaging Polarimetry
100%
Near-infrared
66%
Spherical Grains
66%
Polarization Pattern
66%
Refractive Index
33%
Flux Distribution
33%
Scattered Light Distribution
33%
Strong Dispersion
33%
Three-class
33%
Throwing
33%
Shift-and-add
33%
Interstellar Grains
33%
Disk-shaped
33%
Polarimetry
33%
Wavelength Dependence
33%
Amorphous Carbon
33%
Opacity
33%
Empirical Constraint
33%
Albedo
33%
Elongated Grains
33%
Grain Mixture
33%
Density Distribution
33%
Dark Clouds
33%
Multiple Scattering Model
33%
Taurus
33%
Distribution Pattern
33%
Quadrupolar
33%
Monte Carlo Simulation
33%
High-resolution
33%
Law
33%
Symmetric Density
33%
Scattering Function
33%
Magnetic Clouds
33%
Degree of Circular Polarization
33%
Non-magnetic
33%
Power Law
33%
Dust Grains
33%
Circumstellar Dust
33%
Circumstellar Envelopes
33%
Near-infrared Imaging
33%
Degree of Linear Polarization
33%
Spherically Symmetric
33%
Graphite
33%
Physics
Young Stellar Objects
100%
Polarimetry
100%
Near Infrared
100%
Interstellar Dust
33%
Magnetic Clouds
33%
Monte Carlo Method
33%
Albedo
33%
Refractivity
33%
High Resolution
33%
Dark Interstellar Clouds
33%
Circumstellar Dust
33%
Density Distribution
33%
Earth and Planetary Sciences
Polarimetry
100%
Albedo
33%
Magnetic Clouds
33%
Refractivity
33%
Power Law
33%
Density Distribution
33%
Scattering Function
33%
Circular Polarization
33%
Linear Polarization
33%