2013/10/09 by P. Maggi, F. Haberl, P. J. Kavanagh +12
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Galaxy #Large Magellanic Cloud #Near-Earth supernova #Physics #Radio Astronomy Observations and Technology #Supernova #Supernova remnant #astro-ph.HE
paper · pdf · doi:10.1051/0004-6361/201322820
published as A&A 561, A76, January 2014 · 19 pages, 10 colour Figures, 3 Tables; submitted to Astronomy and Astrophysics
arxiv created 2013/10/09 · openalex publication_date 2013/11/19 · arxiv updated 2014/01/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Aims. We present a detailed multi-wavelength study of four new supernova remnants (SNRs) in the Large Magellanic Cloud (LMC). The objects were identified as SNR candidates in X-ray observations performed during the survey of the LMC with XMM-Newton.