Angular size of the Orion-KL linearly polarized H2O-maser flare region

Details Angular size of the Orion-KL linearly polarized H2O-maser flare region Angular size of the Orion-KL linearly polarized H2O-maser flare region

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..456m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, July-Aug. 1983, p. 456-460) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, July-

Astronomy and Astrophysics

Astronomy

2

Interstellar Masers, Linear Polarization, Orion Nebula, Radio Bursts, Radio Sources (Astronomy), Water Masers, Angular Distribution, Centimeter Waves, Flare Stars, Radial Velocity

Scientific paper

The angular size of the linearly polarized H2O-maser flare region in the Kleinmann-Low nebula has been measured with the Simeiz-Pushchino radio interferometer. The radial velocity of the flare zone is 8 km/sec. A (75 x 100-Gm) ellipse is emitting the central part of the line profile, with a somewhat larger region producing the high-frequency wing. The linear polarization p = 0.5-0.7. The unpolarized region is 1.5-2.0 times as large as the polarized emission zone.

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