Molecular Gas around Symbiotic Miras: Masers in R Aquarii and H1-36

Details Molecular Gas around Symbiotic Miras: Masers in R Aquarii and H1-36 Molecular Gas around Symbiotic Miras: Masers in R Aquarii and H1-36

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..255i&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 255-258

Astronomy and Astrophysics

Astrophysics

6

Masers, R Aquarii, H1-36, Agb Stars

Scientific paper

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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