The Small-scale Structure of N103B - Nature of Nuture?

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dc.creatorLewis, Karen T.
dc.creatorBurrows, David N.
dc.creatorHughes, John P.
dc.creatorSlane, Patrick
dc.creatorGarmire, Gordon P.
dc.creatorNousek, John A.
dc.date2001-08-24
dc.date.accessioned2026-07-07T01:59:45Z
dc.date.available2026-07-07T01:59:45Z
dc.descriptionWe present new results from a 40.8 ks Chandra ACIS observation of the young supernova remnant (SNR) N103B located in the Large Magellanic Cloud. The high resolution Chandra image reveals structure at the sub-arcsecond level, including several bright knots and filaments. Narrow-band imaging and spatially resolved spectroscopy reveal dramatic spectral variations in this remnant as well. In this paper we discuss whether these variations are due to inhomogeneities in the surrounding environment or were generated in the explosion which created the SNR.
dc.description6 pages, 5 figures, in "X-rays at Sharp Focus: Chandra Science Symposium", July 16-18, 2001
dc.identifierhttps://arxiv.org/abs/astro-ph/0108396
dc.identifierhttp://arxiv.org/abs/astro-ph/0108396
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3237
dc.subjectAstrophysics
dc.titleThe Small-scale Structure of N103B - Nature of Nuture?
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