AN INVESTIGATION OF THE ORIGIN OF SOFT X-RAY EXCESS EMISSION FROM Ark 564 AND Mrk 1044
- Author
- DEWANGAN, G. C1 ; GRIFFITHS, R. E1 ; DASGUPTA, Surajit2 ; RAO, A. R2
[1] Department of Physics, Carnegie Mellon University, 5000 Forbes Avenue, Pittsburgh, PA 15213, United States
[2] Department of Astronomy and Astrophysics, Tata Institute of Fundamental Research, Mumbai, 400005, India - Source
The Astrophysical journal. 2007, Vol 671, Num 2, pp 1284-1296, 13 p ; 1 ; ref : 1/2 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
- X-rays: galaxies accretion, accretion disks galaxies: active
- Keyword (fr)
- Disque accrétion Emission RX Galaxies RX Galaxies actives Rayon X mou Source RX cosmique
- Keyword (en)
- Accretion disks X ray emission X-ray galaxies Active galaxies Soft X radiation Cosmic x-ray sources
- Keyword (es)
- Emisión RX
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 19953911
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
10.1086/523683 
https://dx.doi.org/10.1086/523683
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