2022MNRAS.512.2034Y

We investigated the detailed plasma condition of the North Polar Spur (NPS)/Loop I using archival Suzaku data. In previous research, collisional ionization equilibrium (CIE) have been assumed for X-ray plasma state, but we also assume non-equilibrium ionization (NEI) to check the plasma condition in more detail. We found that most of the plasma in the NPS/Loop I favors the state of NEI, and has the density-weighted ionization timescale of n_et ∼ 10^11–12 s cm^–3 and the electron number density n_e ∼ a few x 10^–3 cm^–3. The plasma shock age, t, or the time elapsed after the shock front passed through the plasma, is estimated to be on the order of a few Myr for the NPS/Loop I, which puts a strict lower limit to the age of the whole NPS/Loop I structure. We found that NEI results in significantly higher temperature and lower emission measure than those currently derived under CIE assumption. The electron temperature under NEI is estimated to be as high as 0.5 keV toward the brightest X-ray NPS ridge at Δθ = -20^*, which decreases to 0.3 keV at -10^*, and again increases to ∼0.6 keV towards the outer edge of Loop I at Δθ ∼ 0^*, about twice the currently estimated temperatures. Here, Δθ is the angular distance from the outer edge of Loop I. We discuss the implication of introducing NEI for the research in plasma states in astrophysical phenomena.