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

@article{Knies2021MultiwavelengthAO,
  title={Multiwavelength analysis of the X-ray spur and southeast of the Large Magellanic Cloud},
  author={J. Knies and Manami Sasaki and Yasuo Fukui and K. Tsuge and Frank Haberl and Sean D. Points and Patrick J. Kavanagh and Miroslav D. Filipovi'c},
  journal={Astronomy and Astrophysics},
  year={2021}
}
Aims. The giant H ii 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 H i 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 (∼ 1 kpc) south of 30 Dor called the X-ray spur, which appears to be anticorrelated with the H i gas. We study the properties of the hot interstellar medium… 
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