The association of OH and methanol masers in W3(OH)
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...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2005-07, Vol.360 (3), p.1162-1170 |
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description | 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. |
doi_str_mv | 10.1111/j.1365-2966.2005.09130.x |
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J. ; Gray, M. D.</creator><creatorcontrib>Etoka, S. ; Cohen, R. J. ; Gray, M. D.</creatorcontrib><description>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. 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J.</creatorcontrib><creatorcontrib>Gray, M. D.</creatorcontrib><title>The association of OH and methanol masers in W3(OH)</title><title>Monthly notices of the Royal Astronomical Society</title><addtitle>Mon. Not. R. Astron. Soc</addtitle><description>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.</description><subject>Astronomy</subject><subject>Gases</subject><subject>ISM: individual: W3(OH)</subject><subject>Magnetic fields</subject><subject>masers</subject><subject>Methanol</subject><subject>polarization</subject><subject>radio lines: ISM</subject><subject>Radio telescopes</subject><subject>stars: formation</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2005</creationdate><recordtype>article</recordtype><recordid>eNqNkEFLwzAYhoMoOKf_IQiKHlq_NE3SHjzIcE6YDqSiePnIshQ7u1aTDee_N3Wi4Mkc8gXyPG_CSwhlELOwzuYx41JESS5lnACIGHLGIV5vkd7PxTbpAXARZYqxXbLn_RwAUp7IHuHFs6Xa-9ZUelm1DW1LOhlR3czowi6fddPWdKG9dZ5WDX3gJ5PR6T7ZKXXt7cH37JP74WUxGEXjydX14GIcGSEEREqHpxWwUk5havOZ1NwosEIyDSkkmmdgExMQmyXCmBk3-TSVuQyjVEaUvE-ON7mvrn1bWb_EReWNrWvd2HblMclCvMhlAA__gPN25ZrwN0xA8TQTYe-TbAMZ13rvbImvrlpo94EMsKsS59g1hl1j2FWJX1XiOqhH3_naG12XTjem8r--zJRMUwjc-YZ7r2r78e98vLm9607BjzZ-5Zd2_eNr94JScSVw9PiERV4wNhxzFPwTNHeSYA</recordid><startdate>200507</startdate><enddate>200507</enddate><creator>Etoka, S.</creator><creator>Cohen, R. 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D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c5550-7a966701f6b0be9d6a3c70e561a0402a380e2c667e825ccd3c9b4696c9bf7c5f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2005</creationdate><topic>Astronomy</topic><topic>Gases</topic><topic>ISM: individual: W3(OH)</topic><topic>Magnetic fields</topic><topic>masers</topic><topic>Methanol</topic><topic>polarization</topic><topic>radio lines: ISM</topic><topic>Radio telescopes</topic><topic>stars: formation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Etoka, S.</creatorcontrib><creatorcontrib>Cohen, R. J.</creatorcontrib><creatorcontrib>Gray, M. D.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Solid State and Superconductivity Abstracts</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Etoka, S.</au><au>Cohen, R. J.</au><au>Gray, M. D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The association of OH and methanol masers in W3(OH)</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><addtitle>Mon. Not. R. Astron. Soc</addtitle><date>2005-07</date><risdate>2005</risdate><volume>360</volume><issue>3</issue><spage>1162</spage><epage>1170</epage><pages>1162-1170</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><coden>MNRAA4</coden><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><cop>Oxford, UK</cop><pub>Blackwell Science Ltd</pub><doi>10.1111/j.1365-2966.2005.09130.x</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Astronomy Gases ISM: individual: W3(OH) Magnetic fields masers Methanol polarization radio lines: ISM Radio telescopes stars: formation |
title | The association of OH and methanol masers in W3(OH) |
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