The Evolving XUV Absorber in NGC3516

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dc.creatorMathur, Smita
dc.creatorWilkes, Belinda
dc.creatorAldcroft, Thomas
dc.date1996-08-01
dc.date.accessioned2026-07-07T02:21:42Z
dc.date.available2026-07-07T02:21:42Z
dc.descriptionFor NGC3516 we find that the X-ray warm absorption and the broad UV associated absorption features can be produced by the same absorbing material. We argue that the evolution of the XUV absorber from pre-1992 to 1995 is consistent with expectation for an expanding, outflowing material.
dc.description2 pages, 1 figure. Uses aspconf.sty, included. To be published in the Proceedings of IAU Colloquium 159 on "Emission Lines in Active Galaxies: New Methods and Techniques"
dc.identifierhttps://arxiv.org/abs/astro-ph/9608007
dc.identifierhttp://arxiv.org/abs/astro-ph/9608007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10599
dc.subjectAstrophysics
dc.titleThe Evolving XUV Absorber in NGC3516
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