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Matches in SemOpenAlex for { <https://semopenalex.org/work/W2015451105> ?p ?o ?g. }

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• W2015451105 abstract "We present high-resolution Chandra observations of the remnant of SN 1987A in the Large Magellanic Cloud. The high angular resolution of the Chandra X-Ray Observatory permits us to resolve the X-ray remnant. We find that the remnant is shell-like in morphology, with X-ray peaks associated with some of the optical hot spots seen in Hubble Space Telescope images. The X-ray light curve has deviated from the linear flux increase observed by ROSAT, with a 0.5-2.0 keV luminosity of 1.5 × 1035 ergs s-1 in 2000 January. We set an upper limit of 2.3 × 1034 ergs s-1 on the observed luminosity of any embedded central source (0.5-2 keV). We also present a high-resolution spectrum and show that the X-ray emission is thermal in origin and is dominated by highly ionized species of O, Ne, Mg, and Si." @default.
• W2015451105 created "2016-06-24" @default.
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• W2015451105 date "2000-11-10" @default.
• W2015451105 modified "2023-10-17" @default.
• W2015451105 title "The X-Ray Remnant of SN 1987A" @default.
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• W2015451105 doi "https://doi.org/10.1086/317271" @default.
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