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RADIO CONTINUUM OBSERVATIONS OF THE CANDIDATE SUPERMASSIVE BLACK HOLE IN THE DWARF ELLIPTICAL VCC 128

Author
BUYLE, Pieter1 ; DE RIJCKE, Sven1 ; DEBATTISTA, Victor P2 ; FERRERAS, Ignacio3 ; PASQUALI, Anna4 ; SETH, Anil5 ; MORELLI, Lorenzo6
[1] Sterrenkundig Observatorium, Universiteit Gent, Krijgslaan 281, S9, 9000, Ghent, Belgium
[2] Centre For Astrophysics University of Central Lancashire, Preston PR 2HE, United Kingdom
[3] Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, United Kingdom
[4] Max-Planck-Institut für Astronomie, Koenigstuhl 17, 69117 Heidelberg, Germany
[5] Harvard-Smithsonian Center for Astrophysics, 60 Garden Street MS20, Cambridge, MA 02138, United States
[6] Dipartimento di Astronomia, Universita' di Padova, Vic. Osservatorio 3, 35122 Padova, Italy
Source

The Astrophysical journal. 2008, Vol 685, Num 2, pp 915-918, 4 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
galaxies: dwarf galaxies: individual (VCC 128) galaxies: nuclei radio continuum: galaxies
Keyword (fr)
Continuum Cosmologie Galaxies naines Noyau galaxies Observation radio Radiogalaxies Radiosource cosmique Trou noir supermassif
Keyword (en)
Continuum Cosmology Dwarf galaxies Galaxy nuclei Radio observation Radio galaxies Cosmic radio sources Supermassive black hole
Keyword (es)
Continuo Observación radio Agujero negro supermasivo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20738572

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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