Gas and dust in high redshift quasars

Details Gas and dust in high redshift quasars Gas and dust in high redshift quasars

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.577..115c&link_type=abstract

In: Proceedings of the dusty and molecular universe: a prelude to Herschel and ALMA, 27-29 October 2004, Paris, France. Ed. by A

Physics

10

Quasars, Dust Emission, Molecular Gas, Star Formation

Scientific paper

We review recent progress in the study of dust and gas in optically luminous, radio-quiet high-z quasars (QSOs). Highlights include the detection of thermal dust continuum in ~80 1 < z < 6.4 quasars, and molecular line data in 11 of them including J1148+5152, the farthest known QSO at z = 6.42, indicating the presence of massive reservoirs of dust and molecular gas. The importance of ALMA and Herschel in these studies is underlined.

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