The image reveals a wealth of details that are only possible by combining the power of both space telescopes. It includes a bounty of galaxies outside the cluster and a sprinkling of sources that vary over time, likely due togravitational lensing– the distortion and...
The signal reduction|| frequency distortion happens at a quantum level for each occurrence, and so is not detectable until passage through millions of LY of Dark Matter. Support for this alternate supposition is reasoned from the fact that the M31 Galaxy and the NGC 300 Galaxy are at distances...
It is found that a significant distortion to the structure of the Galactic HI disk will be induced by the collision if the mass of the dwarf exceeds ... RA Ibata,AO Razoumov - arXiv 被引量: 34发表: 1998年 The Dynamics of the Circumnuclear Disk and its environment in the Galactic Cen...
Since halo volume is determined by galactic mass, it must remain constant, implying the distortion of colliding halo boundaries analogous to the collision of two spherical balloons. A dynamical model must consider the diffusion of matter across a changing halo boundary. A new, observable phenomenon ...
Using a more relaxed cluster, Mendygral and collaborators [243] performed MHD simulations confirming the distortion of the morphology of jets and lobes due to the ICM weather. Finally, the recent work by Bourne and Sijacki [244] (using a moving-mesh code) shows that the large-scale ...