The angular structure and intraday variability of a water vapor maser in IC 10

Details The angular structure and intraday variability of a water vapor maser in IC 10 The angular structure and intraday variability of a water vapor maser in IC 10

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...422..586a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 422, no. 2, p. 586-596

Astronomy and Astrophysics

Astronomy

20

Angular Distribution, Irregular Galaxies, Luminosity, Luminous Intensity, Radio Astronomy, Radio Spectra, Water Masers, Centimeter Waves, Interstellar Matter, Scattering, Superhigh Frequencies, Very Large Array (Vla), Very Long Base Interferometry

Scientific paper

The water vapor maser associated with the southeastern nucleus of the irregular galaxy IC 10 has been observed with a six-station intercontinental Very Long Baseline Interferometry (VLBI) array over 3 epochs spanning the period 1990 November to 1991 November. The absolute position of the maser and the relative positions of six spectral features were measured. These features are all unresolved and smaller than approximately 1015 cm (based on a distance of 1.25 Mpc) and have brightness temperatures greater than 3 x 1013 K. The angular distribution of features indicates a region of activity approximately 0.06 pc across. Features of disparate velocity are also clustered on a scale of 1015 cm, similar to Galactic masers. We found the brightest spectral feature reached an integrated luminosity of approximately 0.4 solar luminosity, assuming isotropic emission of radiation. Single-dish observations made in late 1992 and early 1993 suggest that this feature has recently become much stronger, with an integrated luminosity approaching 3 solar luminosity. In addition, we found that one of the features decreased by approximately 60% in flux density over an interval of 17 hr during our VLBI experiment. This is the first intraday variation of an H2O maser witnessed at many telescopes simultaneously. Systematic, although less dramatic variations were observed on timescales of approximately 1 hr. Separate Very Large Array (VLA) observations show that the maser is coincident with a radio continuum source that is smaller than 0.6 pc. We discuss the constraints on possible emission mechanisms imposed by the high luminosity and rapid time variability. We also show that the intraday variation could have been caused by an extreme scattering event due to a cloud in the Galactic interstellar medium (ISM).

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