Active Galactic Nuclei and their role in Galaxy Formation and Evolution

dc.creatorKraemer, Steve
dc.creatorWindhorst, Rogier
dc.creatorCarpenter, Kenneth G.
dc.creatorCrenshaw, Mike
dc.creatorElvis, Martin
dc.creatorKarovska, Margarita
dc.date2009-04-24
dc.date.accessioned2026-07-07T13:08:29Z
dc.date.available2026-07-07T13:08:29Z
dc.descriptionThere are several key open questions as to the nature and origin of AGN including: 1) what initiates the active phase, 2) the duration of the active phase, and 3) the effect of the AGN on the host galaxy. Critical new insights to these can be achieved by probing the central regions of AGN with sub-mas angular resolution at UV/optical wavelengths. In particular, such observations would enable us to constrain the energetics of the AGN "feedback" mechanism, which is critical for understanding the role of AGN in galaxy formation and evolution. These observations can only be obtained by long-baseline interferometers or sparse aperture telescopes in space, since the aperture diameters required are in excess of 500 m - a regime in which monolithic or segmented designs are not and will not be feasible and because these observations require the detection of faint emission near the bright unresolved continuum source, which is impossible from the ground, even with adaptive optics. Two mission concepts which could provide these invaluable observations are NASA's Stellar Imager (SI; Carpenter et al. 2008 & http://hires.gsfc.nasa.gov/si/) interferometer and ESA's Luciola (Labeyrie 2008) sparse aperture hypertelescope.
dc.descriptionWhitepaper submitted to the 2010 Astronomy and Astrophysics Decadal Survey
dc.identifierhttps://arxiv.org/abs/0904.3875
dc.identifierhttp://arxiv.org/abs/0904.3875
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/228431
dc.subjectInstrumentation and Methods for Astrophysics
dc.subjectCosmology and Nongalactic Astrophysics
dc.titleActive Galactic Nuclei and their role in Galaxy Formation and Evolution
dc.typetext

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