Interferometric observations of the mainline OH maser emission from OH127.8-0.0

Details Interferometric observations of the mainline OH maser emission from OH127.8-0.0 Interferometric observations of the mainline OH maser emission from OH127.8-0.0

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.216p...1d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 216, Sept. 1, 1985, p. 1P-5P.

Astronomy and Astrophysics

Astronomy

6

Hydroxyl Emission, Interferometry, Masers, Radio Astronomy, Astronomical Maps, Infrared Stars, Pumping

Scientific paper

The authors have observed the 1667-MHz OH maser emission from OH127.8-0.0 using MERLIN in its spectral line mode. By combining these data with previous MERLIN observations of the 1612-MHz emission they are able to study in detail the relationship between the extended structures at the two frequencies. The structure observed is generally consistent with existing theories of maser pumping, although the lack of any mainline emission inside the well-defined eastern arc of 1612-MHz emission is difficult to explain.

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