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

被引:23
作者
Etoka, S [1 ]
Cohen, RJ
Gray, MD
机构
[1] Univ Manchester, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England
[2] Univ Manchester, Sch Phys & Astron, Manchester M60 1QD, Lancs, England
关键词
magnetic fields; masers; polarization; stars : formation; ISM : individual : W3(OH); radio lines : ISM;
D O I
10.1111/j.1365-2966.2005.09130.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 similar 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.
引用
收藏
页码:1162 / 1170
页数:9
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