Supermassive Black Hole Research in the Post-HST Era

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dc.creatorFerrarese, Laura
dc.date2002-07-01
dc.date.accessioned2026-07-07T02:04:08Z
dc.date.available2026-07-07T02:04:08Z
dc.descriptionThanks to its unprecedented spatial resolution, the Hubble Space Telescope has ended a 20-year long stalemate by detecting the dynamical signature of nuclear supermassive black holes (SBHs) in a sizeable number of nearby galaxies. These detections have revealed the existence of a symbiotic relationship between SBHs and their hosts, changing the way we view SBH and galaxy formation. In this contribution I review which are the most pressing outstanding issues in SBH research, and what are the technological requirements needed to address them.
dc.descriptionInvited contribution to the "Hubble Science Legacy Workshop", held in Chicago, 2-5 April 2002. ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0207050
dc.identifierhttp://arxiv.org/abs/astro-ph/0207050
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4634
dc.subjectAstrophysics
dc.titleSupermassive Black Hole Research in the Post-HST Era
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