Multiwavelength analysis of the X-ray spur and southeast of the Large Magellanic Cloud

Understand

Aims: The giant HII region 30 Doradus (30 Dor) located in the eastern part of the Large Magellanic Cloud is one of the most active star-forming regions in the Local Group.

• Studies of HI data have revealed two large gas structures which must have collided with each other in the region around 30 Dor.
• In X-rays there is extended emission ($\sim 1$ kpc) south of 30 Dor called the X-ray spur, which appears to be anticorrelated with the HI gas.
• We study the properties of the hot interstellar medium (ISM) in the X-ray spur and investigate its origin including related interactions in the ISM.