Author: Richard Carl Bignell
Publisher: c1972.
ISBN:
Category : Polarization (Light)
Languages : en
Pages : 186
Book Description
Polarization of Extragalactic Radio Sources at Centimeter Wavelengths
Author: Richard Carl Bignell
Publisher: c1972.
ISBN:
Category : Polarization (Light)
Languages : en
Pages : 186
Book Description
Publisher: c1972.
ISBN:
Category : Polarization (Light)
Languages : en
Pages : 186
Book Description
Polarization Measurements of Extragalactic Radio Sources at 3.12 Cm Wavelength. 2
Author: G. L. Berge
Publisher:
ISBN:
Category :
Languages : en
Pages : 23
Book Description
The two-element interferometer at the Owens Valley Radio Observatory was used in late 1967 to measure the integrated polarization, both linear and circular, of 32 extragalactic radio sources at a wavelength of 3.12 cm. In addition, flux densities of 103 radio sources were also measured. (Author).
Publisher:
ISBN:
Category :
Languages : en
Pages : 23
Book Description
The two-element interferometer at the Owens Valley Radio Observatory was used in late 1967 to measure the integrated polarization, both linear and circular, of 32 extragalactic radio sources at a wavelength of 3.12 cm. In addition, flux densities of 103 radio sources were also measured. (Author).
The Physics of Extragalactic Radio Sources
Author: David De Young
Publisher: University of Chicago Press
ISBN: 9780226144153
Category : Science
Languages : en
Pages : 588
Book Description
Extragalactic radio sources are among the most unusual and spectacular objects in the universe, with sizes in excess of millions of light years, radiated energies over ten times those of normal galaxies, and a unique morphology. They reveal some of the most dramatic physical events ever seen and provide essential clues to the basic evolutionary tracks followed by all galaxies and groups of galaxies. In The Physics of Extragalactic Radio Sources, David De Young provides a clearly written overview of what is currently known about these objects. A unique feature of the book is De Young's emphasis on the physical processes associated with extragalactic radio sources: their evolution, their environment, and their use as probes to solve other astrophysical problems. He also makes extensive use of the large amount of data now available from observations at x-ray, optical, and radio wavelengths to illustrate his main points. The Physics of Extragalactic Radio Sources will be a comprehensive introduction to the field for graduate students and a useful summary for astrophysicists.
Publisher: University of Chicago Press
ISBN: 9780226144153
Category : Science
Languages : en
Pages : 588
Book Description
Extragalactic radio sources are among the most unusual and spectacular objects in the universe, with sizes in excess of millions of light years, radiated energies over ten times those of normal galaxies, and a unique morphology. They reveal some of the most dramatic physical events ever seen and provide essential clues to the basic evolutionary tracks followed by all galaxies and groups of galaxies. In The Physics of Extragalactic Radio Sources, David De Young provides a clearly written overview of what is currently known about these objects. A unique feature of the book is De Young's emphasis on the physical processes associated with extragalactic radio sources: their evolution, their environment, and their use as probes to solve other astrophysical problems. He also makes extensive use of the large amount of data now available from observations at x-ray, optical, and radio wavelengths to illustrate his main points. The Physics of Extragalactic Radio Sources will be a comprehensive introduction to the field for graduate students and a useful summary for astrophysicists.
Observations of the Flux Density and Linear Polarization of Compact Extragalactic Radio Sources at 3.7- and 11.1-cm Wavelength
Author: Daniel R. Altschuler
Publisher:
ISBN:
Category : Polarization (Light)
Languages : en
Pages : 67
Book Description
Publisher:
ISBN:
Category : Polarization (Light)
Languages : en
Pages : 67
Book Description
THE POLARIZATION OF RADIO SOURCES AT 3.75 CENTIMETER WAVELENGTH.
Author: ROBERT WESLEY HOBBS
Publisher:
ISBN:
Category :
Languages : en
Pages : 261
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 261
Book Description
The Polarization of Radio Sources at 3.75 Centimeter Wavelength
Author: R.W. Hobbs
Publisher:
ISBN:
Category :
Languages : en
Pages : 248
Book Description
Publisher:
ISBN:
Category :
Languages : en
Pages : 248
Book Description
Extragalactic Radio Sources
Author: David Michael Mills
Publisher:
ISBN:
Category : Radio sources (Astronomy)
Languages : en
Pages : 100
Book Description
Publisher:
ISBN:
Category : Radio sources (Astronomy)
Languages : en
Pages : 100
Book Description
The Linear Polarization of Radio Sources I
Author: F. F. Gardner
Publisher:
ISBN:
Category : Radio sources (Astronomy)
Languages : en
Pages : 36
Book Description
Publisher:
ISBN:
Category : Radio sources (Astronomy)
Languages : en
Pages : 36
Book Description
The Polarization of Extragalactic Radio Sources
Author: John Patrick Leahy
Publisher:
ISBN:
Category : Radio sources (Astronomy)
Languages : en
Pages : 165
Book Description
Publisher:
ISBN:
Category : Radio sources (Astronomy)
Languages : en
Pages : 165
Book Description
The Linear Polarization of Radio Sources Between 11 and 20 Cm Wavelength. Iii. Influence of the Galaxy on Source Depolarization and Faraday Rotation
Author: F. F. Gardner
Publisher:
ISBN:
Category :
Languages : en
Pages : 7
Book Description
The dependence on galactic latitude of the 11 and 20 cm polarization of 355 extragalactic sources reveals no definite evidence of depolarization within the Galaxy. The distribution of Faraday rotation can be explained in terms of a field along the local spiral arm, deformed by magnetic 'loops' in the solar neighbourhood. (Author).
Publisher:
ISBN:
Category :
Languages : en
Pages : 7
Book Description
The dependence on galactic latitude of the 11 and 20 cm polarization of 355 extragalactic sources reveals no definite evidence of depolarization within the Galaxy. The distribution of Faraday rotation can be explained in terms of a field along the local spiral arm, deformed by magnetic 'loops' in the solar neighbourhood. (Author).