Projected XMM Vision for MCVs

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dc.creatorJames, Cynthia H.
dc.creatorBranduardi-Raymont, Graziella
dc.creatorCropper, Mark
dc.date1998-09-24
dc.date.accessioned2026-07-07T02:28:03Z
dc.date.available2026-07-07T02:28:03Z
dc.descriptionThe XMM satellite has a scientific payload of 3 EPIC and 2 RGS instruments which provide for both imaging and non-dispersive spectroscopy as well as medium-to-high resolution dispersive spectroscopy, in the soft to medium X-ray bands. The co-aligned OM adds the facility for simultaneous optical and UV studies. In this poster paper we describe the instrumental characteristics of XMM, comparing them to those of ASCA. We also forecast the expected X-ray spectra of a selection of both the Polars and Intermediate Polars by means of simulations based on ASCA model fits.
dc.descriptionTo be published in Proc Annapolis workshop on magnetic CVs, held in July 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9809316
dc.identifierhttp://arxiv.org/abs/astro-ph/9809316
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12953
dc.subjectAstrophysics
dc.titleProjected XMM Vision for MCVs
dc.typetext

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