No CrossRef data available.
Article contents
First detection of Zeeman splitting of water masers in circumstellar shells
Published online by Cambridge University Press: 03 August 2017
Abstract
The strength and structure of the magnetic fields in circumstellar envelopes have been measured through polarization observations of OH and SiO masers. Here we present the first results obtained by observing the circular polarization of the H2O masers using VLBI. SiO masers are probes of the high temperature and density regime close to the central star. OH masers are found at much lower densities and temperatures, generally much further out in the circumstellar envelope. The detection of the Zeeman splitting of the (616-523) rotational transition of the H2O maser allows us to determine the magnetic field strength in the intermediate temperature and density regime.
- Type
- Part 4. Polarization and Magnetic Fields
- Information
- Symposium - International Astronomical Union , Volume 206: Cosmic Masers: From Protostars to Blackholes , 2002 , pp. 375 - 378
- Copyright
- Copyright © Astronomical Society of the Pacific 2002