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Monitoring the bidirectional relativistic jets of the radio galaxy 3C 338

Author
GENTILE, G1 ; RODRIGUEZ, C1 2 ; TAYLOR, G. B1 3 ; GIOVANNINI, G4 5 ; ALLEN, S. W6 ; LANE, W. M7 ; KASSIM, N. E7
[1] Department of Physics and Astronomy, University of New Mexico, Albu querque, NM 87131, United States
[2] Department of Physics, Universidad Simon Bolivar, Sartenejas, Venezuela
[3] National Radio Astronomy Observatory, Socorro, NM 87801, United States
[4] Dipartimento di Astronomia, Universita' di Bologna, 40127 Bologna, Italy
[5] Istituto di Radioastronomia-INAF, 40129 Bologna, Italy
[6] Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94305-4060, United States
[7] Naval Research Laboratory, Washington, DC 20375, United States
Source

The Astrophysical journal. 2007, Vol 659, Num 1, pp 225-234, 10 p ; 1 ; ref : 1/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
University of Chicago Press, Chicago, IL
Publication country
United States
Document type
Article
Language
English
Author keyword
distance scale galaxies: active galaxies: individual (3C 338) galaxies: jets radio continuum: galaxies
Keyword (fr)
Continuum Echelle distance Galaxies actives Jet relativiste Radiogalaxies Radiosource cosmique
Keyword (en)
Continuum Distance scale Active galaxies Relativistic jet Radio galaxies Cosmic radio sources
Keyword (es)
Continuo Escala distancia Chorro relativista
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
18701371

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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