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Fifty Years of Quasars: Current Impressions and Future Perspectives

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Fifty Years of Quasars

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 386))

Abstract

Contributors to the previous chapters describe an impressive body of research carried out over the past 50 years. One can argue that there is now considerable evidence supporting the hypothesis that the quasar phenomenon is driven by accretion onto a supermassive object. Hard X-ray emission may be the most direct signature of that accretion process and perhaps the only universal property shared by all types of AGN. This possibility brings us closer to an operational definition of the quasar phenomenon and therefore may answer the question posed in the Introduction.

Contributions by Jack W. Sulentic, Paola Marziani, and Mauro D’Onofrio

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Notes

  1. 1.

    ESA—Space Science News: Raging storms sweep away galactic gas, May 9, 2011.

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Authors and Affiliations

  1. Instituto de Astrofísica de Andalucía (CSIC), Granada, Spain

    Jack W. Sulentic

  2. INAF, Osservatorio Astronomico di Padova, Vicolo Osservatorio 5, IT35122, Padova, Italy

    Paola Marziani

  3. Dipartimento di Astronomia, Università degli Studi di Padova, Vicolo Osservatorio 3, I35122, Padova, Italy

    Mauro D’Onofrio

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  1. , Dipartimento di Astronomia, Università di Padova, Vicolo Osservatorio 3, Padova, 35122, Italy

    Mauro D'Onofrio

  2. , Osservatorio Astronomico di Padova, Istituto Nazionale di Astrofisica (INAF), Vicolo dell' Osservatorio 5, Padova, 35122, Italy

    Paola Marziani

  3. , (IAA-CSIC), Instituto de Astrofisica de Andalucia, Camino Bajo del Huetor 50, Granada, 18008, Spain

    Jack W. Sulentic

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Sulentic, J.W., Marziani, P., D’Onofrio, M. (2012). Fifty Years of Quasars: Current Impressions and Future Perspectives. In: D'Onofrio, M., Marziani, P., Sulentic, J. (eds) Fifty Years of Quasars. Astrophysics and Space Science Library, vol 386. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27564-7_9

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