GTThe high Galactic latitude 3/4 keV background consists of both extragalactic and Galactic emission with uncertain relative contributions. The spectrum at3/4 keV shows an excess over the extrapolatio
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...
