Radio and Gamma-ray Evidence for the Supernova Origin of High Velocity Cloud Complex M
Joan T. Schmelz, Gerrit L. Verschuur

TL;DR
This study presents evidence linking a supernova explosion approximately four million years ago to the formation of high velocity cloud Complex M and the Local Chimney, using radio and gamma-ray observations.
Contribution
It identifies a supernova remnant as the origin of high velocity cloud Complex M through multi-wavelength data analysis and energetic calculations.
Findings
Detected a cavity in radio data coinciding with gamma-ray minima.
Estimated the supernova explosion energy at 3.0 ± 1.0 × 10^{50} ergs.
Determined the explosion occurred about four million years ago.
Abstract
Using -21-cm galactic neutral atomic hydrogen data from the HI4PI survey of Bekhti et al. (2016) and 0.75-30 MeV -ray emission from the Imaging Compton Telescope, we have searched for the origin event that accelerated high velocity cloud Complex M. Radio plots of , , and show a cavity centered at (, ) (150, 50.) and extending about 33. The best view of the cavity is at a velocity of -25 km s, which shows a circular cross section on the back (receding) face. Complex M, at -85 km s, is on the front (approaching) face. The -ray emission reveals several minima, the largest centered at (, ) (150, 50.) and coincident with the position and extent of the cavity seen in the radio data. Using the know distance to Complex M and assuming that the cavity is…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena
