Cosmic Feedback from Supermassive Black Holes

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dc.creatorFabian, A.
dc.creatorChurazov, E.
dc.creatorDonahue, M.
dc.creatorForman, W. R.
dc.creatorGarcia, M. R.
dc.creatorHeinz, S.
dc.creatorMcNamara, B. R.
dc.creatorNandra, K.
dc.creatorNulsen, P.
dc.creatorOgle, P.
dc.creatorPerlman, E. S.
dc.creatorProga, D.
dc.creatorRees, M. J.
dc.creatorSarazin, C. L.
dc.creatorSunyaev, R. A.
dc.creatorTaylor, G. B.
dc.creatorWhite, S. D. M.
dc.creatorVikhlinin, A.
dc.creatorWorrall, D. M.
dc.date2009-03-25
dc.date.accessioned2026-07-07T12:56:33Z
dc.date.available2026-07-07T12:56:33Z
dc.descriptionAn extraordinary recent development in astrophysics was the discovery of the fossil relationship between central black hole mass and the stellar mass of galactic bulges. The physical process underpinning this relationship has become known as feedback. The Chandra X-ray Observatory was instrumental in realizing the physical basis for feedback, by demonstrating a tight coupling between the energy released by supermassive black holes and the gaseous structures surrounding them. This white paper discusses how a great leap forward in X-ray collecting area and spectral resolution will allow a qualitatively new way of studying how feedback from black holes influenced the growth of structure.
dc.descriptionScience white paper submitted to the Astro2010 Decadal Survey
dc.identifierhttps://arxiv.org/abs/0903.4424
dc.identifierhttp://arxiv.org/abs/0903.4424
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/224619
dc.subjectCosmology and Nongalactic Astrophysics
dc.subjectHigh Energy Astrophysical Phenomena
dc.titleCosmic Feedback from Supermassive Black Holes
dc.typetext

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