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Are quasars dustyTwo separate techniques have been applied to estimate the amount of dust in the line of sight toward a number of quasars. No evidence for dust was found. Estimates of the dust-to-gas ratio in the emission-line region of quasars suggest that it is much less than the value in our Galaxy. These results provide strong evidence against dust theories of the infrared emission from quasars. The possible relationship between quasars and galaxies is discussed. Finally, a new upper limit on the dust content of the intergalactic medium is obtained.
Document ID
19740047285
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mckee, C. F.
(Harvard College Observatory and Smithsonian Astrophysical Observatory Cambridge, Mass., United States)
Petrosian, V.
Date Acquired
August 7, 2013
Publication Date
April 1, 1974
Publication Information
Publication: Astrophysical Journal
Volume: 189
Subject Category
Space Sciences
Accession Number
74A30035
Funding Number(s)
CONTRACT_GRANT: NGR-05-020-510
Distribution Limits
Public
Copyright
Other

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