Results 81 to 90 of about 3,094 (200)
Spectropolarimetry provides a unique probe of ejecta asphericities, offering direct insights into the underlying explosion physics of Type Ia supernovae (SNe Ia).
Aleksandar Cikota +8 more
doaj +1 more source
Spatially resolved measurement of helium atom emission line spectrum in scrape-off layer of Heliotron J by near-infrared Stokes spectropolarimetry. [PDF]
Chatani T +18 more
europepmc +1 more source
Spectropolarimetry of FIRST 0840 + 3633 [PDF]
We present Keck spectropolarimetry of a rare ``Iron Lo- BALQSO,`` FIRST 0840+3633. The continuum is {approximately}4% polarized near 2000{Angstrom} rest-frame, but falls to {approximately}2% at longer wavelengths, and maintains a relatively constant ...
Brotherton, M.S. +3 more
core
The geometry and morphology of symbiotic stars (SySts) are conducive to a variety of scattering phenomena. Among the most prominent is the Raman scattering of the O VI doublet λλ 1032, 1038, which often shows strongly polarized features in the visible ...
Arijit Maiti +2 more
doaj +1 more source
Snapshot Mueller spectropolarimeter imager. [PDF]
Dai T +6 more
europepmc +1 more source
X-Ray Polarization Study of the Neutron Star Low-mass X-Ray Binary GX 349+2
We report the first X-ray polarimetric results of the neutron star (NS) low-mass X-ray binary Z-source GX 349+2 using the Imaging X-ray Polarimetry Explorer (IXPE). We discovered that the X-ray source was polarized at a polarization degree of PD = 1.1% ±
Unnati Kashyap +5 more
doaj +1 more source
Novel developments in computational spectropolarimeter. [PDF]
Hsiang EL, Wu ST.
europepmc +1 more source
Testing spectropolarimetry in the extreme ultraviolet to infer the solar coronal magnetic field
Context. Spectropolarimetry has the potential to provide us with important coronal plasma parameters. Aims. We test spectropolarimetric forward modelling by investigating whether it is possible to reproduce the only linear polarisation ...
A. Khan
core +1 more source
Energy-dependent Polarization Angle Variability as a Robust Diagnostic for Blazar Flaring Mechanisms
Identifying the physical mechanism driving blazar flares remains a central challenge in high-energy astrophysics. We show that the energy dependence of the standard deviation of the polarization angle variability ( σ _PA ) provides a powerful and robust ...
Haocheng Zhang +4 more
doaj +1 more source
We have carried out spectropolarimetric observations of the Wolf-Rayet star WR66 (WN8) with EFOSC1 mounted on the ESO 3.6m telescope of La Silla. The results indicate a polarization level of about 5 to 6 % in the continuum which is most probably due to interstellar polarization.
Lamy, H. +2 more
openaire +1 more source

