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Giant metrewave radio telescope observations of the 2006 outburst of the nova RS ophiuchi : First detection of emission at radio frequencies <1.4 GHz

Author
KANTHARIA, N. G1 ; ANUPAMA, G. C2 ; PRABHU, T. P2 ; RAMYA, S2 ; BODE, M. F3 ; EYRES, S. P. S4 ; O'BRIEN, T. J5
[1] National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Post Bag 3, Ganeshkhind, Pune 411 007, India
[2] Indian Institute of Astrophysics, Koramangala, Bangalore 560 034, India
[3] Astrophysics Research Institute, Liverpool John Moores University, Birkenhead CH41 ILD, United Kingdom
[4] Centre for Astrophysics, University of Central Lancashire, Preston PR1 2HE, United Kingdom
[5] School of Physics and Astronomy, Jodrell Bank Observatory, University of Manchester, Macclesfield SK 11 9DL, United Kingdom
Source

The Astrophysical journal. 2007, Vol 667, Num 2 ; L171-L174 ; 2 ; 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
binaries : close novae, cataclysmic variables radio continuum: stars stars: individual (RS Ophiuchi)-supernovae: general
Keyword (fr)
Binaire serrée Continuum Emission radioélectrique Etoile radio Etoile variable cataclysmique Nova Observation radio Supernova
Keyword (en)
Close binary stars Continuum Radio emission Radio stars Cataclysmic variable stars Novae Radio observation Supernovae
Keyword (es)
Continuo Emisión radioeléctrica Observación radio
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
19135980

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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