EUSO-Balloon is a pathfinder for JEM-EUSO, the Extreme Universe Space Observatory which is to be hosted on-board the International Space Station. As JEM-EUSO is...
We report 323 hours of nearly uninterrupted time series photometric observations of the DBV star GD 358 acquired with the Whole Earth Telescope (WET) during May...
The Evershed Effect Observed with 0.2" Angular Resolution
We present an analysis of the Evershed effect observed with a resolution of 0.2". Using the new Swedish 1 m Solar Telescope and its Littrow spectrograph, we...
The evolution of a supernova remnant in a strongly magnetized interstellar medium
Several aspects of the evolution of an SNR into a low-beta ISM are investigated. The presence of a strong magnetic field in the unperturbed ISM is found to have...
The Evolution of AGN Activity in Brightest Cluster Galaxies
We present the results of an analysis of Wide-field Infrared Survey Explorer (WISE) observations of the full 2500 deg 2 South Pole Telescope (SPT)-Sunyaev-Zel...
The evolution of compact massive quiescent and star-forming galaxies derived from the R<SUB>e</SUB>-R<SUB>h</SUB> and M<SUB>star</SUB>-M<SUB>h</SUB> relations
The mean size (effective radius R e) of massive galaxies (MGs; M star > 10 11.2M ⊙) is observed to increase steadily with cosmic time. It is still unclear...
The evolution of compact supernova remnants in a strongly magnetized medium
Two-dimensional simulations of the evolution of supernova remnants in a uniform, high-density medium are presented. The medium is magnetized, and its magnetic...
The evolution of early-type galaxies in clusters from z˜ 0.8 to z ˜ 0: the ellipticity distribution and the morphological mix
We present the ellipticity distribution and its evolution for early-type galaxies in clusters from z˜ 0.8 to the current epoch, based on the WIde-field Nearby...