Astronomy and Astrophysics – Astronomy
Scientific paper
May 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986mnras.220..513c&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 220, May 15, 1986, p. 513-528.
Astronomy and Astrophysics
Astronomy
142
Radio Astronomy, Stellar Envelopes, Supergiant Stars, Hydroxyl Emission, Power Spectra, Radial Velocity, Stellar Magnetic Fields, Stellar Structure, Water Masers
Scientific paper
MERLIN maps of the H2O and OH maser emission from the circumstellar envelope of the supergiant star VX Sagittarius are presented. The OH masers at 1612 MHz are at a radial distance of 2 x 10 to the 16th cm from the star and lie in a 'thin-shell' region which has an expansion velocity of about 19 km/s. The H2O masers occur nearer the star in an accelerating 'thick-shell' region which has a mean radius of about 3 x 10 to the 15th cm and a mean expansion velocity of about 9 km/s. The OH mainline masers have angular and velocity extents similar to those of the H2O masers and are believed to lie in the same thick shell, although absolute position measurements are needed to confirm this. The distribution of masers in this inner region is asymmetric. This may be due to the influence of the stellar magnetic field. The magnetic field in the envelope is determined from Zeeman splitting of the OH mainlines to be about 2 mG. The velocity field of the circumstellar envelope as traced by SiO, H2O and OH maser lines cannot be driven by a 1/R-squared radiation pressure law with constant dust opacity. It is suggested that the driving force per unit mass increases outwards to a distance of at least 50 stellar radii.
Chapman Jessica M.
Cohen Richard J.
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