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The Polarized Water Maser in Orion

Published online by Cambridge University Press:  07 August 2017

Z. Abraham  and
J.W.S. Vilas Boas
Z. Abraham
Affiliation:
IAG/USP, CP 9638, CEP 04301, São Paulo, SP, Brazil
J.W.S. Vilas Boas
Affiliation:
CRAAE/PTR, CP 8174, 05588, São Paulo, SP, Brazil

Abstract

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We present the results of 12 years of observations of the 8 km s−1 water maser in Orion. Four large flares in the flux density were observed, as well as variability in the degree and angle of polarization. The profile of the line is also variable, indicating the superposition of several sources.

Type
Quiescent Clouds and Regions of Star Formation
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 275 - 276
Copyright
Copyright © Kluwer 1992 

References

REFERENCES

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