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The association of OH and methanol masers in W3(OH).

Authors :
Etoka, S.
Cohen, R. J.
Gray, M. D.
Source :
Monthly Notices of the Royal Astronomical Society. 7/1/2005, Vol. 360 Issue 3, p1162-1170. 9p.
Publication Year :
2005

Abstract

We present single-baseline Multi-Element Radio-Linked Interferometer Network (MERLIN) measurements of excited OH 6.0-GHz masers and methanol 6.7-GHz masers for the source W3(OH). These allow us to compare the positions of individual maser spots of these two species to∼15 mas accuracy for the first time, and to compare these with previously published positions of ground-state OH masers near 1.7 GHz and excited-state OH masers near 4.7 GHz. There is a strong association between OH 6035-MHz and 1665-MHz masers. OH and methanol have very similar distributions, but associations of individual masers are relatively rare: most methanol 6.7-GHz masers are within 100 mas of OH 6.0-GHz masers, but only four methanol masers are within 15 mas of an OH 6.0-GHz maser. There are no correspondences of either species with excited OH 4.7-GHz masers. Zeeman splitting of the 6.0-GHz OH lines indicates an ordered magnetic field ranging from 3.2 to 14.4 mG. The magnetic fields estimated from co-propagating masers such as 6035 and 1665 MHz are generally in good agreement with each other. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
360
Issue :
3
Database :
Academic Search Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
17304080
Full Text :
https://doi.org/10.1111/j.1365-2966.2005.09130.x