Multi-frequency study of supernova remnants in the Large Magellanic Cloud

2012/07/30 by P. Maggi, F. Haberl, L. M. Bozzetto +14 · 1 citation
Physics and Astronomy · #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Astrophysics and Cosmic Phenomena #Context (archaeology) #Gamma-ray bursts and supernovae #Infrared #Large Magellanic Cloud #Optics #Physics #Radiation #Spectral index #Spectral line #Star formation #Stars #Supernova #Supernova remnant #Wavelength #Young stellar object #astro-ph.GA #astro-ph.HE

paper · pdf · doi:10.1051/0004-6361/201219708

published as Astronomy and Astrophysics, Volume 546, A109, October 2012 · 11 pages, 6 figures, accepted for publication in A&A

openalex publication_date 2012/07/30 · arxiv created 2012/08/01 · arxiv updated 2012/10/17 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The Large Magellanic Cloud (LMC) is an ideal target for the study of an unbiased and complete sample of supernova remnants (SNRs). We started an X-ray survey of the LMC with XMM-Newton, which, in combination with observations at other wavelengths, will allow us to discover and study remnants that are either even fainter or more evolved (or both) than previously known.

Citations

• Dust Destruction in Fast Shocks of Core-Collapse Supernova Remnants in the Large Magellanic Cloud
• Catalogues of Hα-EMISSION Stars and Nebulae in the Magellanic Clouds.
• H I in the Galaxy
• The Second Survey of the Molecular Clouds in the Large Magellanic Cloud by NANTEN. I. Catalog of Molecular Clouds
• The Formation of Constellation III in the Large Magellanic Cloud

Cited by

• Multi-frequency study of DEM L299 in the Large Magellanic Cloud