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Optical spectra of compact objects.On the basis of their optical spectra, compact objects are divided into three classes: (1) nonthermal objects including Seyfert nuclei, most N-type radio galaxies, and luminous Zwicky objects; (2) hot massive stars, and (3) stellar objects including some compact galaxies having only absorption line spectra. A variety of morphological forms exist among class (1) and (2) objects. Emission line spectra of quasars are reviewed and related to the physical conditions in the emitting regions.
Document ID
19720032706
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Burbidge, E. M.
(California, University San Diego, Calif.; Cambridge University, Cambridge, United Kingdom)
Date Acquired
August 6, 2013
Publication Date
January 1, 1972
Subject Category
Space Sciences
Meeting Information
Meeting: External galaxies and quasi-stellar objects;Symposium, University of Uppsala
Location: Uppsala
Country: Sweden
Start Date: August 10, 1970
End Date: August 14, 1970
Accession Number
72A16372
Funding Number(s)
CONTRACT_GRANT: NGL-05-005-004
Distribution Limits
Public
Copyright
Other

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