If the disappearance of the broad emission lines observed in changing-look quasars originates from the obscuration of the quasar core by dusty clouds moving in...
Polarization of Photospheric Lines from Turbulent Dynamo Simulations
We employ the magnetic and velocity fields from turbulent dynamo simulations to synthesize the polarization of a typical photospheric line. The synthetic Stokes...
Polarization of the changing-look quasar J1011+5442
If the disappearance of the broad emission lines observed in changing-look quasars were caused by the obscuration of the quasar core through moving dust clouds...
Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the...
Polarization of the Lyα Lines of H I and He II as a Tool for Exploring the Solar Corona
The near-Earth space weather is driven by the quick release of magnetic free energy in the solar corona. Probing this extremely hot and rarified region of the...
Polarization properties of changing-look active galactic nuclei: NGC 1365 and NGC 2992
Changing-look active galactic nuclei (CLAGNs) represent a rare class of AGNs that undergo transitions from type 1 (characterized by the presence of broad...
Polarization-correction device with liquid crystals for quantum-key-distribution satellite systems
In this paper, we present a device, designed to be used in a space payload, capable of correcting any arbitrary polarization state. The device consists of a set...
Polarized infrared emission from X-ray binary jets
Near-infrared (NIR) and optical polarimetric observations of a selection of X-ray binaries are presented. The targets were observed using the Very Large...
Polarized Mid-infrared Synchrotron Emission in the Core of Cygnus A
We present high-angular (~0.''4) resolution mid-infrared (MIR) polarimetric observations in the 8.7 μm and 11.6 μm filters of Cygnus A using CanariCam on the 10...