High resolution radio images of the symbiotic system R aquarii

S. M. Dougherty, M. F. Bode, H. M. Lloyd, R. J. Davis, S. P. Eyres

Allbwn ymchwil: Cyfraniad at gyfnodolynErthygladolygiad gan gymheiriaid

1 Dyfyniad (Scopus)

Crynodeb

We present MERLIN images of the symbiotic system R Aquarii obtained at 1.7 and 5 GHz. We identify the emission from the binary system and derive a mass loss rate for the Mira that is commensurate with that in typical Miras. We show that variations in the radio emission over the last decade are consistent with the jet model for the system originally presented by Solf (1992). In addition, we calculate the spectral index distribution and find that there is no evidence of non-thermal emission.

Iaith wreiddiolSaesneg
Tudalennau (o-i)453-454
Nifer y tudalennau2
CyfnodolynAstrophysics and Space Science
Cyfrol224
Rhif cyhoeddi1-2
Dynodwyr Gwrthrych Digidol (DOIs)
StatwsCyhoeddwyd - Chwef 1995

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