Abstract
The concept of studying symbiotic Miras via their molecular emission holds the promise of an improved understanding of the circumbinary environment in symbiotics, but following the largely ineffective maser surveys conducted during the 1970s and 80s there has been a widespread misconception that this avenue of study is a dead end. Here, we present spectral line and continuum maps of R Aqr and H1—36, two objects in which OH and H2O masers were detected during a recent survey of symbiotic Miras.
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References
Allen, D.A., Hall, P.J., Norris, R.P., Troup, E.R., Wark, R.M., Wright, A.E.: 1989, Mon. Not. of the RAS 236, 363.
Hall, P.J., Wright, A.E., Troup, E.R., Wark, R.M., Allen, D.A.: 1990, Mon. Not. of the RAS 247, 549.
Ivison, R.J., Seaquist, E.R. and Hall, P.J.: 1994, Mon. Not. of the RAS 269, 218.
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© 1995 Springer Science+Business Media Dordrecht
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Ivison, R.J., Seaquist, E.R., Hall, P.J. (1995). Molecular Gas around Symbiotic Miras: Masers in R Aquarii and H1-36. In: Watt, G.D., Williams, P.M. (eds) Circumstellar Matter 1994. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0147-9_43
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DOI: https://doi.org/10.1007/978-94-011-0147-9_43
Publisher Name: Springer, Dordrecht
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