FOREVER22: galaxy formation in protocluster regions
We present results from a new cosmological hydrodynamics simulation campaign of protocluster (PC) regions, FOREVER22: FORmation and EVolution of galaxies in...
Formation and morphology of anomalous solar circular polarization
Context. The morphology of spectral line polarization is the most valuable observable to investigate the magnetic and dynamic solar atmosphere. However, in...
Formation of polarized spectral lines in atmospheres with horizontal inhomogeneities
We study the problem of the generation and transfer of spectral line intensity and polarization in models of stellar atmospheres with horizontal plasma...
Full Stokes-vector Inversion of the Solar Mg II h and k Lines
The polarization of the Mg II h and k resonance lines is the result of the joint action of scattering processes and the magnetic field–induced Hanle, Zeeman...
G5T: ExoMolHD: Precision spectroscopic data for studies of exoplanets and other hot atmospheres
The ExoMol project ( www.exomol.com) provides comprehensive spectroscopic data (line lists) for the study of atmospheres of exoplanets and other hot bodies...
Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure-driven...
Gauss-Seidel and Successive Overrelaxation Methods for Radiative Transfer with Partial Frequency Redistribution
The linearly polarized solar limb spectrum that is produced by scattering processes contains a wealth of information on the physical conditions and magnetic...
Height Variation of the Vector Magnetic Field in Solar Spicules
Proving the magnetic configuration of solar spicules has hitherto been difficult due to the lack of spatial resolution and image stability during off-limb...
Herschel-ATLAS: The dust energy balance in the edge-on spiral galaxy UGC 4754
We use Herschel PACS and SPIRE observations of the edge-on spiral galaxy UGC 4754, taken as part of the H-ATLAS SDP observations, to investigate the dust energy...