North Polar Spur/Loop I: gigantic outskirt of the Northern Fermi bubble or nearby hot gas cavity blown by supernovae?
Rosine Lallement

TL;DR
This paper reviews the longstanding debate over the nature of Loop I/NPS, analyzing recent multi-wavelength data and proposing a hybrid scenario that combines local and distant origins, highlighting the need for further data.
Contribution
It synthesizes recent observational results and proposes a new hybrid model for Loop I/NPS, bridging the gap between conflicting theories.
Findings
No single scenario fully explains all data
Recent observations challenge purely local or distant origins
A hybrid model may reconcile different constraints
Abstract
Radio continuum, microwave and gamma-ray images of the Milky Way reveal a conspicuous, loop-like structure that fills almost half of the northern Galactic hemisphere, called Loop I. The interior of Loop I is shining in soft X-rays, and its eastern base is a bright, elongated structure dubbed the North Polar Spur (NPS). After 40 years of debates, two contradictory views of Loop I/NPS are still defended: on the one hand, the NPS is a volume of expanding hot gas that envelops and extends the northern Fermi Bubble (FB) known to be blown by the Galactic center, and Loop I marks the shock front; on the other hand, the NPS is a nearby cavity of hot gas blown by supernovae, Loop I is its shock front and they are coincidentally located in the direction of the FB. To an observer at the Sun, both structures can produce the same perspective view, although the former has a size comparable to the…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomy and Astrophysical Research · Stellar, planetary, and galactic studies
