A Spatially Resolved Study of X-Ray Properties in Superbubble 30 Dor C with XMM-Newton

We carry out a spatially resolved spectral analysis with a physical scale of ∼10 pc in X-ray for the superbubble 30 Dor C, which has the largest diameter of ∼80 pc and the brightest non-thermal emission in superbubbles, for the first time. We aim at investigating spatial variation of the physical properties of non-thermal emission as detected in some supernova remnants in order to study particle acceleration in a superbubble. We demonstrated that non-thermal components are detected in all the regions covering the entire field of 30 Dor C. The spectra in the west region of 30 Dor C can be described with a combination of the thermal and non-thermal components, while the spectra in the east region can be fitted with the non-thermal component alone. The photon index and absorption-corrected intensity in 2-10 keV of the non-thermal component show spatial variation from ∼2.0 to ∼3.7 and (4-130) × 10^-8 erg s^-1 cm^-2 str^-1, respectively, and the negative correlation between the non-thermal physical properties is observed. The temperature and normalization of the thermal component also vary within a range of ∼0.2-0.3 keV and ∼(0.2-7) × 10¹⁷ cm^-5 str^-1, respectively, and the positive correlation between the photon index and the normalization is also detected. We revealed the correlations in a supperbubble for the first time as is the case in supernova remnants, which suggests the possibility that the same acceleration mechanism works also in the supperbubble.