An investigation of SNRs in the magellanic clouds-SNR B0450-708 and SNR B0455-687

Details An investigation of SNRs in the magellanic clouds-SNR B0450-708 and SNR B0455-687 An investigation of SNRs in the magellanic clouds-SNR B0450-708 and SNR B0455-687

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..429f&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 429-432 (2001).

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Supernova Remnants, Magellanic Clouds And Other Irregular Galaxies, Pulsars

Scientific paper

We are studying the nature and the spatial distribution of ~80 supernova remnants (SNRs) in the Magellanic Clouds (MCs). A multi-frequency comparison of these sources involves the latest radio, IR, optical and X-ray surveys with angular resolution of ~1'. Their morphology, birth rate and overall properties are investigated and compared with SNRs in our Galaxy and other galaxies. In this paper we are presenting initial results from two SNRs in the Large Magellanic Cloud (LMC). .

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