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MASERS IN SPACE
Of the seven molecules presently detected at radio wavelengths in the interstellar medium, OH and H₂O display spectacular emission properties attributed to maser action. The OH masers fall into three distinct classes, herein described, each of which is anomalously excited by a different pumping mech...
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Published in: | Publications of the Astronomical Society of the Pacific 1970-10, Vol.82 (489), p.996-1021 |
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container_title | Publications of the Astronomical Society of the Pacific |
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creator | TURNER, B. E. |
description | Of the seven molecules presently detected at radio wavelengths in the interstellar medium, OH and H₂O display spectacular emission properties attributed to maser action. The OH masers fall into three distinct classes, herein described, each of which is anomalously excited by a different pumping mechanism. Far IR radiative pumping is applied to recent observations of anomalous OH emission in dust clouds. The excitation of OH by the collisional dissociation of water vapor is described next, and is shown to explain recent observations of microwave emission from excited states of OH. It also explains why the type of OH emission that it produces (Class I) is observed to occur in the same regions as anomalous H₂O emission. A pumping mechanism for the H₂O is also described which is expected to operate in any regions in which Class I OH emission occurs. |
doi_str_mv | 10.1086/128997 |
format | article |
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E.</creator><creatorcontrib>TURNER, B. E.</creatorcontrib><description>Of the seven molecules presently detected at radio wavelengths in the interstellar medium, OH and H₂O display spectacular emission properties attributed to maser action. The OH masers fall into three distinct classes, herein described, each of which is anomalously excited by a different pumping mechanism. Far IR radiative pumping is applied to recent observations of anomalous OH emission in dust clouds. The excitation of OH by the collisional dissociation of water vapor is described next, and is shown to explain recent observations of microwave emission from excited states of OH. It also explains why the type of OH emission that it produces (Class I) is observed to occur in the same regions as anomalous H₂O emission. 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A pumping mechanism for the H₂O is also described which is expected to operate in any regions in which Class I OH emission occurs.</description><subject>Cosmic dust</subject><subject>Ground state</subject><subject>Hydroxyl radical clouds</subject><subject>Hydroxyl sources</subject><subject>Infrared radiation</subject><subject>Main lines</subject><subject>Masers</subject><subject>Molecules</subject><subject>Photons</subject><subject>Pumping</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1970</creationdate><recordtype>article</recordtype><recordid>eNo9j0tLxDAUhYMoWMfHLxBm5S56b26SJstSqg6MD6yuSx5zwUEZaWbjv7dSEQ6cxfk48AlxjnCN4OwNKud9fSAqNOQkuZoORQUAWlrl4FiclLIFQHQIlbh4aPrupV-uHpf9c9N2p-KIw0fZnP31Qrzddq_tvVw_3a3aZi2TIr2XTIlD5JCsUcnqmhXH7DKoFK1jjGxdyGQsB4iE4Kc5-UzZ5ynBRFqIq_k3jbtSxg0PX-P7Zxi_B4ThV2OYNSbwcga3Zb8b_ykNtrZGK_oBcIRA1w</recordid><startdate>19701001</startdate><enddate>19701001</enddate><creator>TURNER, B. E.</creator><general>The Astronomical Society of the Pacific</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19701001</creationdate><title>MASERS IN SPACE</title><author>TURNER, B. E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c234t-f3cfabfac652c647f2fbd8d02cb68f1bf68ad356fa0b31092fbc9d3d9dd9da5b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1970</creationdate><topic>Cosmic dust</topic><topic>Ground state</topic><topic>Hydroxyl radical clouds</topic><topic>Hydroxyl sources</topic><topic>Infrared radiation</topic><topic>Main lines</topic><topic>Masers</topic><topic>Molecules</topic><topic>Photons</topic><topic>Pumping</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>TURNER, B. E.</creatorcontrib><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>TURNER, B. E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>MASERS IN SPACE</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1970-10-01</date><risdate>1970</risdate><volume>82</volume><issue>489</issue><spage>996</spage><epage>1021</epage><pages>996-1021</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>Of the seven molecules presently detected at radio wavelengths in the interstellar medium, OH and H₂O display spectacular emission properties attributed to maser action. The OH masers fall into three distinct classes, herein described, each of which is anomalously excited by a different pumping mechanism. Far IR radiative pumping is applied to recent observations of anomalous OH emission in dust clouds. The excitation of OH by the collisional dissociation of water vapor is described next, and is shown to explain recent observations of microwave emission from excited states of OH. It also explains why the type of OH emission that it produces (Class I) is observed to occur in the same regions as anomalous H₂O emission. A pumping mechanism for the H₂O is also described which is expected to operate in any regions in which Class I OH emission occurs.</abstract><pub>The Astronomical Society of the Pacific</pub><doi>10.1086/128997</doi><tpages>26</tpages><oa>free_for_read</oa></addata></record> |
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source | JSTOR Archival Journals and Primary Sources Collection; Institute of Physics:Jisc Collections:IOP Publishing Read and Publish 2024-2025 (Reading List) |
subjects | Cosmic dust Ground state Hydroxyl radical clouds Hydroxyl sources Infrared radiation Main lines Masers Molecules Photons Pumping |
title | MASERS IN SPACE |
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