Rotation measure of the H2O maser flare region in Orion-KL

Details Rotation measure of the H2O maser flare region in Orion-KL Rotation measure of the H2O maser flare region in Orion-KL

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..199m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Mar. 1984, p. 199-202) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Mar.-Apr

Astronomy and Astrophysics

Astronomy

1

Interstellar Masers, Maser Outputs, Orion Nebula, Spectral Line Width, Water Masers, Faraday Effect, Polarized Radiation

Scientific paper

Measurements in October, 1983, indicate that the polarization angle of the H2O-maser emission in the Kleinmann-Low nebula varies over the line profile by 0.5 deg/kHz. The rotation measure is estimated to be 5.3 x 10 to the 8th rad/sq m. The integrated flare emission, whose line halfwidth is 47.7 kHz, is depolarized by only a few percent. Linearly polarized maser emission in the 18-cm OH lines is not observable in Orion-KL.

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