Please use this identifier to cite or link to this item: http://cmuir.cmu.ac.th/jspui/handle/6653943832/61629
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dc.contributor.authorS. Nammahachaken_US
dc.contributor.authorK. Asanoken_US
dc.contributor.authorB. Hutawarakorn Krameren_US
dc.contributor.authorR. J. Cohenen_US
dc.contributor.authorO. Muanwongen_US
dc.contributor.authorN. Gasiprongen_US
dc.date.accessioned2018-09-11T08:56:14Z-
dc.date.available2018-09-11T08:56:14Z-
dc.date.issued2006-09-01en_US
dc.identifier.issn13652966en_US
dc.identifier.issn00358711en_US
dc.identifier.other2-s2.0-33748684602en_US
dc.identifier.other10.1111/j.1365-2966.2006.10740.xen_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=33748684602&origin=inwarden_US
dc.identifier.urihttp://cmuir.cmu.ac.th/jspui/handle/6653943832/61629-
dc.description.abstractMulti-Element Radio-Linked Interferometer Network polarization measurements of the OH 18-cm masers in ON1 are presented. OH maser emission is detected in all four ground state lines. The bulk of the masers lie in an elongated distribution covering 2 arcsec at position angle 130°, near the southern edge of the ultracompact H II region. The maser distribution is orthogonal to the bipolar outflow seen in HCO + at position angle (PA) 44°. An isolated group of 1720-MHz masers is also seen 6 arcsec to the east. The magnetic field deduced from Zeeman splitting of the OH maser lines shows a large-scale order, with field values ranging from -0.4 to -4.6 mG. © 2006 RAS.en_US
dc.subjectEarth and Planetary Sciencesen_US
dc.subjectPhysics and Astronomyen_US
dc.titleOH masers associated with bipolar outflow in ON1en_US
dc.typeJournalen_US
article.title.sourcetitleMonthly Notices of the Royal Astronomical Societyen_US
article.volume371en_US
article.stream.affiliationsKhon Kaen Universityen_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsUniversity of Manchesteren_US
article.stream.affiliationsUbon Rajathanee Universityen_US
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