Very Long Baseline Interferometry of 1720 MHz masers in W3(OH)

Astronomy and Astrophysics – Astronomy

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H Ii Regions, Hydroxyl Emission, Interstellar Masers, Radio Astronomy, Star Formation, Astronomical Models, Emission Spectra, Methyl Alcohol, Power Spectra, Very Long Base Interferometry

Scientific paper

Results are reported from 5-station intercontinental VLBI observations of 1720 MHz OH masers in W3(OH). Two regions of maser emission were detected, superimposed on northern and southern parts of the H II region. Maser spots are individually unresolved and are less than or equal to 1.2 mas Full Width at Half Maximum (FWHM), placing an upper limit on interstellar scattering. These observations show that 1720 MHz maser spots are significantly smaller than 1665 MHz spots. Using a maser model described in Gray et al. (1992), the data are analyzed in terms of an accelerating and outflowing zone in the northern region, where 1720, 4765 and 1665 MHz maser spots may be spatially coincident. Geometrical effects leading to maser beaming in a turbulent medium are also modeled and these effects are sufficient to explain the relative sizes of maser spots at 1720 and 1665 MHz.

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