Hostname: page-component-5c6d5d7d68-vt8vv Total loading time: 0.001 Render date: 2024-08-16T07:57:57.188Z Has data issue: false hasContentIssue false

Multi-Epoch VLBA Observations of the SiO Maser Emission Towards R Aquarii (R Aqr)

Published online by Cambridge University Press:  12 April 2016

D. A. Boboltz
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
P. J. Diamond
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.
A. J. Kemball
Affiliation:
National Radio Astronomy Observatory, Socorro, NM 87801, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have observed ν = 1, J = 1 – 0, 43-GHz SiO maser emission towards the symbiotic Mira variable R Aqr at four different epochs in the stellar pulsation cycle using the VLBA.

Type
Research Article
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Diamond, P.J., et al. 1994. ApJ, 430, L6164.Google Scholar
Kemball, A.J. & Diamond, P.J. 1997. ApJ, 481, Llll114.Google Scholar