New XMM-Newton observations of supernova remnants in the Small Magellanic Cloud

2008/05/02 by M. D. Filipović, M. D. Filipovic, F. Haberl +8 · 2 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Pulsars and Gravitational Waves Research #astro-ph

paper · pdf · doi:10.1051/0004-6361:200809642

8 pages, 6 figures, Accepted for publication in A&A

arxiv created 2008/05/02 · openalex publication_date 2008/05/06 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/07/31

Abstract

Context. A complete overview of the supernova remnant (SNR) population is required to investigate their evolution and interaction with the surrounding interstellar medium in the Small Magellanic Cloud (SMC).

Cited by

• XMM-Newton observations of the Small Magellanic Cloud: Be/X-ray binary pulsars active between October 2006 and June 2007
• IKT 16: a composite supernova remnant in the Small Magellanic Cloud

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