Diffuse X-ray emission from the superbubbles N 70 and N 185 in the Large Magellanic Cloud

Abstract

We present a study of the diffuse X-ray emission from superbubbles N 70 (DEM L301) and N 185 (DEM L25) located in the Large Magellanic Cloud, based on data from the XMM-Newton Satellite. We obtained spectra and images of these objects in the soft X-ray energy band. These X-ray spectra were fitted by a thermal plasma model, with temperatures of $2.6\times 10^6$ K and $2.3\times 10^6$ K, for N 70 and N 185, respectively. For N 70, images show that X-ray emission comes from the inner regions of the superbubble, when we compare the distribution of the X-ray and the optical emission; while for N 185, the X-ray emission is partially confined by the optical shell. We suggest that the observed X-ray emission is caused by shock-heated gas, inside of the optical shells. We also obtained X-ray luminosities which exceed the values predicted by the standard analytical model. This fact shows that, in addition to the winds of the interior stars, it is necessary to consider another ingredient in the description, such as a supernova explosion, as has been proposed in previous numerical models.

arXiv comment9 pages, 7 figures. Accepted for publication in AJ

References in corpus (6)

• The European Photon Imaging Camera on XMM-Newton: The MOS Cameras
• Collisional Plasma Models with APEC/APED: Emission Line Diagnostics of Hydrogen-like and Helium-like Ions
• A Catalog of Galaxy Clusters Observed by XMM-Newton
• ASCA X-Ray Spectroscopy of LMC Supernova Remnants and the Metal Abundances of the LMC
• The XMM-Newton EPIC Background and the production of Background Blank Sky Event Files
• X-ray emission and dynamics from large diameter superbubbles: The case of N 70 superbubble

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• The soft and hard X-rays thermal emission from star cluster winds with a supernova explosion
• Physical properties of superbubbles in the Antennae galaxies
• Understanding the Baryon Cycle: Fueling Star Formation via Inflows in Milky Way-like Galaxies
• Dissecting the hot bubbles in LMC-N57 with XMM-Newton
• H$\alpha$ Kinematics of Superbubbles and Supernova Remnants of the Dwarf galaxy NGC 4214