Radio variability properties for radio sources
- Author
- FAN, J. H1 2 ; LIU, Y1 ; XU, S. X1 ; CHEN, J. L1 ; YUAN, Y. H1 ; HUA, T. X1 ; WANG, H. G1 ; WANG, Y. X3 ; YANG, J. H4 ; GUPTA, A. C5 ; LI, J1 ; ZHOU, J. L1
[1] Center for Astrophysics, Guangzhou University, Guangzhou 510006, China
[2] Physics Institute, Hunan Normal University, Changsha, China
[3] College of Science and Trade, Guangzhou University, Guangzhou 511442, China
[4] Department of Physics and Electronics Science, Hunan University of Arts and Science, Changde 415000, China
[5] Tata Institute of Fundamental Research, Homi Bhabha Road, Colaba, Mumbai -400005, India - Source
Astronomy and astrophysics (Berlin. Print). 2007, Vol 462, Num 2, pp 547-552, 6 p ; ref : 1/4 p
- CODEN
- AAEJAF
- ISSN
- 0004-6361
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Author keyword
- BL lacertae objects: general methods: data analysis quasars: general
- Keyword (fr)
- Analyse donnée Analyse spectrale Corrélation Courbe lumière Densité flux Méthode spectrale Objet BL Lacertae Observatoire radioastronomique Périodicité Quasar Radiosource cosmique Spectre radio Variabilité
- Keyword (en)
- Data analysis Spectral analysis Correlations Light curves Flux density Spectral method BL Lacertae objects Radio astronomy observatory Periodicity Quasars Cosmic radio sources Radio spectrum Variability
- Keyword (es)
- Método espectral Observatorio radioastronómico Periodicidad Espectro radio Variabilidad
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 18454823
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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DOI
10.1051/0004-6361:20054775 
https://dx.doi.org/10.1051/0004-6361:20054775
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