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EVN Observations of the OH megamaser galaxies Mrk 231 and IC 694
Published online by Cambridge University Press: 03 August 2017
Abstract
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We present EVN observations of hydroxyl (OH) main-line emission in two megamaser sources Mrk 231 and IC 694. The observations indicate that the broad maser emission lines originate within the nuclear regions. A single 1667 MHz main-line feature is seen at the nucleus of IC 694. In Mrk 231 both main-lines were observed in an extended “half-circular” region of 150 pc by 50 pc surrounding the radio nucleus.
- Type
- Part 5. Extragalactic Nuclear Masers
- Information
- Symposium - International Astronomical Union , Volume 206: Cosmic Masers: From Protostars to Blackholes , 2002 , pp. 430 - 433
- Copyright
- Copyright © Astronomical Society of the Pacific 2002
References
Diamond, P. J., Lonsdale, C. J., Lonsdale, Ca. J., & Smith, H. E.
1999, ApJ, 511, 178
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