Galaxies are believed to become active by a process where two gas-rich galaxies merge, causing gas inflow to the supermassive black hole, which will then fuel...
Large scale structure - Its possible imprint on the CMB?
The new results of the Jodrell-IAC Cosmic Microwave Background (CMB) anisotropy experiment for declination +40 deg are presented. A similar level of sensitivity...
Large-amplitude longitudinal oscillations in solar prominences
Large-amplitude longitudinal (LAL) prominence oscillations consist of periodic mass motions along a filament axis. The oscillations appear to be triggered by an...
Large-Amplitude Oscillations as a Probe of Solar Prominences
Large-amplitude oscillations in prominences are among the most spectacular phenomena of the solar atmosphere. Such an oscillations involve motions with...
Large-scale radio nebula around the Ultra-Luminous X-ray Source IC 342 X-1
We present discovery of a radio nebula associated with the ultraluminous X-ray source (ULX) IC 342 X-1 using the Very Large Array (VLA). Taking the surrounding...
Large-Scale Star Formation Patterns in Spiral Arms
An observational study of large-scale star formation processes in spiral galaxies with well-defined arm systems is presented. Combining new data on the current...