Published May 1976 | Version v1
Journal article

Refraction effects and position stability in components of the water source W49

Creators

  • 1. Kent Univ., Canterbury (UK)

Description

Long baseline interferometer observations have shown that the relative positions of strong components in the water source W49 (H2O) change by angles approximately 0.05 in periods of a few months (Knowles et al (Astr. J.; 79:925 1974))). Bodily motion of the individual components cannot explain the apparent changes, since this would imply velocities approximately 104 km s-1, which are much too high; a model in which a number of differently situated masers switch independently on and off is statistically improbable. Refraction effects producing 'ghost images', of the type suggested by Gold, cannot account for the possition jitter. Neither, it appears, can inherent instability in the solution of the radiative transfer equations, postulated by Deguchi (Publ. Astr. Soc. Japan; 26:437 (1974)). It is hard to explain the variations of position by stochastic motions of irregularities within the masing clouds, so it seems most likely that changes in the location of the pump energy input to the maser are responsible for the observed behaviour. (author)

Additional details

Identifiers

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
175
Journal Issue
2
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
245-255
ISSN
0035-8711

Optional Information

Notes
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