The radio counterpart of the likely TeV binary HESS J0632+057

Monthly Notices of the Royal Astronomical Society

Volumn 399, Issue 1, 2009, Pages 317-322

  Skilton, J L ^a   Pandey Pommier, M ^b   Hinton, J A ^a   Cheung, C C ^c   Aharonian, F A ^d   Brucker, J ^e   Dubus, G ^f   Fiasson, A ^g,h   Funk, S ⁱ   Gallant, Y ^g   Marcowith, A ^g   Reimer, O ^i,j  

^a UNIVERSITY OF LEEDS   (United Kingdom)

^b LEIDEN UNIVERSITY   (Netherlands)

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^e UNIVERSITY OF ERLANGEN NUREMBERG   (Germany)

^f CNRS   (France)

^g UNIVERSITÉ MONTPELLIER II   (France)

^h CENTRE DE CALCUL DE L INSTITUT NATIONAL DE PHYSIQUE NUCLEAIRE ET DE PHYSIQUE DES PARTICULES   (France)

ⁱ STANFORD UNIVERSITY   (United States)

^j UNIVERSITY OF INNSBRUCK   (Austria)

more..

Author keywords

Radio continuum: stars; X rays: binaries

Indexed keywords

GAMMA RAYS; SYSTEMS (METALLURGICAL); TELLURIUM COMPOUNDS;

BE STARS; BINARY SYSTEMS; GIANT METREWAVE RADIO TELESCOPES; NEW MEMBERS; RADIO CONTINUUM: STARS; SPECTRAL INDICES; STARS: BE; VERY LARGE ARRAYS; X-RAY EMISSION; X-RAYS: BINARIES;

STARS;

EID: 70349671123     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.15272.x     Document Type: Article

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