The ASKAP Variables and Slow Transients survey is designed to search for transient and highly variable sources on timescales from 10 seconds to months and years. The scientific goals are to study phen
Timings of primary eclipse up through 1992 are collected, plus a few overlooked in earlier studies. Analysis shows that, after decreasing until ~1919 and increasing since then,...
We wish to improve our understanding of the Orion central star formation region (Orion-KL) and disentangle its complexity. We collected data with ALMA during cycle 2 in 16GHz of...
