Optical identifications of flat-spectrum radio sources
A complete sample of radio sources with S> or =0.3 Jy at 1400 MHz, +24/sup 0/ or =+0.5 are usually in empty fields. The lower limits that can be assigned to the radio-optical spectral indices ..cap alpha../sub RO/ of these sources are significantly higher than the median ..cap alpha../sub RO/ of the sources with flat high-frequency spectra, so the optical characteristics of the two classes of radio source are intrinsically different. The radio and optical fluxes of flat-spectrum QSO's appear to be correlated, at least when averaged over 10/sup 2/--10/sup 3/ yr.
- Research Organization:
- National Radio Astronomy Observatory, Edgemont Road, Charlottesville, Virginia 22901
- OSTI ID:
- 6527605
- Journal Information:
- Astron. J.; (United States), Journal Name: Astron. J.; (United States) Vol. 88:1; ISSN ANJOA
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640103* -- Astrophysics & Cosmology-- Quasi-Stellar
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COORDINATES
CORRELATIONS
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
FREQUENCY RANGE
GHZ RANGE
GHZ RANGE 01-100
INTERFEROMETRY
QUASARS
RADIATIONS
SPECTRA
VISIBLE RADIATION
Radio
& X-Ray Sources-- (-1987)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
COORDINATES
CORRELATIONS
COSMIC RADIO SOURCES
ELECTROMAGNETIC RADIATION
FREQUENCY RANGE
GHZ RANGE
GHZ RANGE 01-100
INTERFEROMETRY
QUASARS
RADIATIONS
SPECTRA
VISIBLE RADIATION