Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..453d&link_type=abstract
Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 453-454
Astronomy and Astrophysics
Astrophysics
Scientific paper
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.
Bode Michael F.
Davis Raymond Jr.
Dougherty Sean M.
Eyres Stewart P. S.
Lloyd H. M.
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