Evolution of powerful extragalactic radio sources.
Observations of complete flux density limited samples of powerful extragalactic radio sources by very-long-baseline interferometry enable us to study the evolution of these objects over the range of linear scales from 1 parsec to 15 kiloparsees (1 parsec = 3.09 x 10(18) cm). The observations are con...
Gardado en:
| Publicado en: | Proc Natl Acad Sci U S A |
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| Autor Principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado: |
National Academy of Sciences
1995
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| Acceso en liña: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC40418/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/11607616/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.92.25.11447 |
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