Possible connection between the asymmetry of North Polar Spur and Loop I with Fermi Bubbles
Kartick Chandra Sarkar

TL;DR
This paper proposes that the asymmetry of the North Polar Spur and Loop I can be explained by a slight difference in circumgalactic medium density, supporting a common Galactic center origin for these structures and Fermi Bubbles.
Contribution
It demonstrates that small density asymmetries and projection effects can account for observed asymmetries, linking NPS, Loop I, and Fermi Bubbles to a star formation driven wind from the Galactic center.
Findings
Asymmetries explained by 20% lower CGM density in the south.
Estimated FB age of approximately 28 million years.
Consistent mechanical luminosity with star formation driven wind scenario.
Abstract
The origin of North Polar Spur (NPS) and Loop-I has been debated over almost half a century and is still unresolved. Most of the confusion is caused by the absence of any prominent counterparts of these structures in the southern Galactic hemisphere (SGH). This has also led to doubts over the claimed connection between the NPS and Fermi Bubbles (FBs). I show in this paper, that such asymmetries of NPS and Loop-I in both X-rays and -rays can be easily produced if the circumgalactic medium (CGM) density in the southern hemisphere is only smaller by than the northern counterpart in case of a star formation driven wind scenario. The required mechanical luminosity, erg s (reduces to M yr including the non-thermal pressure) and the age of the FBs, Myr, are consistent…
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