A look at SNR 0519-69.0 with Chandra's ACIS

Details A look at SNR 0519-69.0 with Chandra's ACIS A look at SNR 0519-69.0 with Chandra's ACIS

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..185w&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 185-188 (2001).

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Supernova Remnants, Magellanic Clouds And Other Irregular Galaxies, Mass Loss And Stellar Winds

Scientific paper

The young, Balmer-dominated SNR 0519-69.0 in the Large Magellanic Cloud is of the class of objects typified by the Tycho supernova remnant. Recent observations with Chandra's Advanced CCD Imaging Spectrometer have shown the X-ray structure of this object in unprecedented detail. ACIS's combination of spatial and spectral resolution allow us to compare the X-ray spectra of the outermost limb emission to that from the rest of the remnant, revealing intriguing differences in spectral features. .

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