The Very Local Universe in X-rays

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dc.creatorPtak, A.
dc.creatorFeigelson, E.
dc.creatorChu, Y. -H.
dc.creatorKuntz, K.
dc.creatorZezas, A.
dc.creatorSnowden, S.
dc.creatorde Martino, D.
dc.creatorTrinchieri, G.
dc.creatorFabbiano, G.
dc.creatorForman, W.
dc.creatorTagliaferri, G.
dc.creatorGiacconi, R.
dc.creatorMurray, S.
dc.creatorAllen, S.
dc.creatorBautz, M.
dc.creatorBorgani, S.
dc.creatorBrandt, N.
dc.creatorCampana, S.
dc.creatorDonahue, M.
dc.creatorFlannagan, K.
dc.creatorGilli, R.
dc.creatorJones, C.
dc.creatorMiller, N.
dc.creatorPareschi, G.
dc.creatorRosati, P.
dc.creatorSchneider, D.
dc.creatorTozzi, P.
dc.creatorVikhlinin, A.
dc.date2009-02-24
dc.date.accessioned2026-07-07T12:46:39Z
dc.date.available2026-07-07T12:46:39Z
dc.descriptionWhile the exceptional sensitivity of Chandra and XMM-Newton has resulted in revolutionary studies of the Galactic neighborhood in the soft (<10 keV) X-ray band, there are many open questions. We discuss these issues and how they would be addressed by very wide-area (> 100 sq. deg.) X-ray surveys.
dc.description8 pages, Astro2010 Science White paper. Full-resolution version available at http://wfxt.pha.jhu.edu
dc.identifierhttps://arxiv.org/abs/0902.4239
dc.identifierhttp://arxiv.org/abs/0902.4239
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/221453
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleThe Very Local Universe in X-rays
dc.typetext

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