X-ray detection of SN1988Z with the ROSAT HRI

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dc.creatorFabian, A. C.
dc.creatorTerlevich, R.
dc.date1995-11-14
dc.date.accessioned2026-07-07T02:20:25Z
dc.date.available2026-07-07T02:20:25Z
dc.descriptionWe report the detection of SN1988Z in X-rays with the ROSAT High Resolution Imager. The inferred X-ray luminosity of about $10^{41}\ergps$ can be well explained by assuming that the supernova occurred in a dense circumstellar medium, consistent with optical observations. SN1988Z is the most distant supernova yet detected in X-rays.
dc.description4 pages (including figures) uuencoded compressed postscript file. Submitted for publication in Monthly Notices of the Royal Astronomical Society
dc.identifierhttps://arxiv.org/abs/astro-ph/9511060
dc.identifierhttp://arxiv.org/abs/astro-ph/9511060
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10207
dc.subjectAstrophysics
dc.titleX-ray detection of SN1988Z with the ROSAT HRI
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