Results 81 to 90 of about 247 (167)

When Magnetic Fields Sculpt the Sky: The Riegel–Crutcher Cloud in Optical Polarization

open access: yesThe Astrophysical Journal
Filamentary structures are ubiquitous in the interstellar medium, yet the extent to which magnetic fields influence the morphology of cold atomic gas remains an open question.
Gabriel A. P. Franco   +4 more
doaj   +1 more source

Light pollution of freshwater ecosystems: principles, ecological impacts and remedies. [PDF]

open access: yesPhilos Trans R Soc Lond B Biol Sci, 2023
Hölker F   +4 more
europepmc   +1 more source

Synchrotron Polarization of Anisotropic Electron Distribution in GRB Prompt Emission

open access: yesThe Astrophysical Journal
In γ -ray bursts (GRBs), the electron pitch angle ( α ) is usually assumed to be isotropically distributed. However, recent numerical simulations indicate that only the high-energy electrons (with Lorentz factors γ  >  γ _iso ) are distributed ...
Kang-Fa Cheng   +9 more
doaj   +1 more source

The magnetic field of the Radcliffe wave: Starlight polarization at the nearest approach to the Sun

open access: yesAstronomy & Astrophysics
Aims. We investigate the geometry of the magnetic field toward the Radcliffe wave, a coherent part of the nearby Local Arm of 3 kpc in length recently discovered via three-dimensional dust mapping. Methods. We used archival stellar polarization in the optical and new measurements in the near-infrared to trace the magnetic field as projected on the ...
G. V. Panopoulou   +8 more
openaire   +2 more sources

Mapping the Interstellar Magnetic Field Around the Heliosphere with Polarized Starlight

open access: yes, 2018
Starlight that becomes linearly polarized by magnetically aligned dust grains provides a viable diagnostic of the interstellar magnetic field (ISMF). A survey is underway to map the local ISMF using data collected at eight observatories in both hemispheres.
Frisch, P. C.   +22 more
openaire   +2 more sources

B-fields and Dust in Interstellar Filaments Using Dust Polarization (BALLAD-POL). III. Grain Alignment and Disruption Mechanisms in G34.43+0.24 Using Polarization Observations from JCMT/POL-2

open access: yesThe Astrophysical Journal
Polarization of starlight and thermal dust emission due to aligned non-spherical grains helps us to trace magnetic field ( B -field) morphology in molecular clouds and to study grain alignment mechanisms.
Saikhom Pravash   +5 more
doaj   +1 more source

Dust in and Around the Heliosphere and Astrospheres. [PDF]

open access: yesSpace Sci Rev, 2022
Sterken VJ   +9 more
europepmc   +1 more source

Field and intensity correlations: the Siegert relation from stars to quantum emitters. [PDF]

open access: yesEur Phys J D At Mol Opt Phys, 2022
Lassègues P   +11 more
europepmc   +1 more source

B-fields and Dust in Interstellar Filaments Using Dust Polarization (BALLAD-POL). II. Testing the Radiative Torque Paradigm in Musca and OMC-1

open access: yesThe Astrophysical Journal
Polarization of starlight and thermal dust emission caused by aligned dust grains is a valuable tool to characterize magnetic fields ( B -fields) and constrain dust properties. However, the grain alignment physics is not fully understood.
Nguyen Bich Ngoc   +3 more
doaj   +1 more source

High-harmonic generation from a subwavelength dielectric resonator. [PDF]

open access: yesSci Adv, 2023
Zalogina A   +9 more
europepmc   +1 more source

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