Detection of H3+ in the diffuse interstellar medium toward Cygnus OB2 No. 12

The molecular ion H3+ is considered the cornerstone of interstellar chemistry because it initiates the reactions responsible for the production of many larger molecules. Recently discovered in dense molecular clouds, H3+ has now been observed in the diffuse interstellar medium toward Cygnus OB2 No....

Full description

Saved in:
Bibliographic Details
Published in:Science (American Association for the Advancement of Science) 1998-03, Vol.279 (5358), p.1910-1913
Main Authors: MCCALL, B. J, GEBALLE, T. R, HINKLE, K. H, OKA, T
Format: Article
Language:English
Subjects:
Astronomical Phenomena
Astronomy
Atomic, molecular, chemical, and grain processes
Carbon Monoxide
Cations, Monovalent
Chemistry
Cosmic Dust
Cosmic Radiation
Cygnus (Constellation)
Discovery and exploration
Earth, ocean, space
Exact sciences and technology
Extraterrestrial Environment
Interstellar hydrogen
Interstellar medium (ism) and nebulae in milky way
Mathematics
Observations
Organic Chemistry
Space life sciences
Star & galaxy formation
Stellar systems. Galactic and extragalactic objects and systems. The universe
Temperature
Tritium
Vision
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page 1913
container_issue 5358
container_start_page 1910
container_title Science (American Association for the Advancement of Science)
container_volume 279
creator MCCALL, B. J
GEBALLE, T. R
HINKLE, K. H
OKA, T
description The molecular ion H3+ is considered the cornerstone of interstellar chemistry because it initiates the reactions responsible for the production of many larger molecules. Recently discovered in dense molecular clouds, H3+ has now been observed in the diffuse interstellar medium toward Cygnus OB2 No. 12. Analysis of H3+ chemistry suggests that the high H3+ column density (3.8 x 10(14) per square centimeter) is due not to a high H3+ concentration but to a long absorption path. This and other work demonstrate the ubiquity of H3+ and its potential as a probe of the physical and chemical conditions in the interstellar medium.
doi_str_mv 10.1126/science.279.5358.1910
format article
fullrecord <record><control><sourceid>gale_proqu</sourceid><recordid>TN_cdi_proquest_miscellaneous_79741233</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><galeid>A20458362</galeid><sourcerecordid>A20458362</sourcerecordid><originalsourceid>FETCH-LOGICAL-g515t-44195bb564f8177a9996c47bb17c0bac881888617bfbd851fb4def80a72ed92f3</originalsourceid><addsrcrecordid>eNqN0ltrFDEUB_BBlLpWP0IhiKhgZ8x1kjy2q24LS_fBy-uQyZyMKXNpJxlsv30jXYSVRZc8hOT_45DLybITggtCaPkxWA-DhYJKXQgmVEE0wU-yBcFa5Jpi9jRbYMzKXGEpnmcvQrjGOGWaHWVHWuBSs3KRrT9BBBv9OKDRoQv2AfkBxZ-AGu_cHCAtI0whQteZCfXQ-LlHcfxlpgYt79thDmhzTtHVWCBCX2bPnOkCvNrOx9n3L5-_LS_y9WZ1uTxb560gIuacEy3qWpTcKSKl0VqXlsu6JtLi2liliFKqJLJ2daMEcTVvwClsJIVGU8eOs7ePdW-m8XaGEKveB_v7iAOMc6iklpxQxhJ892_IWVkSTcV_S1LClcScJPj6L3g9ztOQrpsME4IryhM6fUSt6aDygxvjZGwLA0ymGwdwPm2fUcyFYiVNPN_D02ig93aff7_jE4lwF1szh1Bdfr06mG5-HEzPV4dStVrv0NN91I5dBy1UqS-Wmx1-sn3euU7dVt1MvjfTfbVt2JS_2eYmWNO5yQzWhz-M0vTxWrIHJtny1w</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>213554824</pqid></control><display><type>article</type><title>Detection of H3+ in the diffuse interstellar medium toward Cygnus OB2 No. 12</title><source>Education Collection (Proquest) (PQ_SDU_P3)</source><source>JSTOR Archival Journals and Primary Sources Collection</source><source>Science Online_科学在线</source><source>Social Science Premium Collection (Proquest) (PQ_SDU_P3)</source><source>Alma/SFX Local Collection</source><creator>MCCALL, B. J ; GEBALLE, T. R ; HINKLE, K. H ; OKA, T</creator><creatorcontrib>MCCALL, B. J ; GEBALLE, T. R ; HINKLE, K. H ; OKA, T</creatorcontrib><description>The molecular ion H3+ is considered the cornerstone of interstellar chemistry because it initiates the reactions responsible for the production of many larger molecules. Recently discovered in dense molecular clouds, H3+ has now been observed in the diffuse interstellar medium toward Cygnus OB2 No. 12. Analysis of H3+ chemistry suggests that the high H3+ column density (3.8 x 10(14) per square centimeter) is due not to a high H3+ concentration but to a long absorption path. This and other work demonstrate the ubiquity of H3+ and its potential as a probe of the physical and chemical conditions in the interstellar medium.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.279.5358.1910</identifier><identifier>PMID: 9506936</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Astronomical Phenomena ; Astronomy ; Atomic, molecular, chemical, and grain processes ; Carbon Monoxide ; Cations, Monovalent ; Chemistry ; Cosmic Dust ; Cosmic Radiation ; Cygnus (Constellation) ; Discovery and exploration ; Earth, ocean, space ; Exact sciences and technology ; Extraterrestrial Environment ; Interstellar hydrogen ; Interstellar medium (ism) and nebulae in milky way ; Mathematics ; Observations ; Organic Chemistry ; Space life sciences ; Star &amp; galaxy formation ; Stellar systems. Galactic and extragalactic objects and systems. The universe ; Temperature ; Tritium ; Vision</subject><ispartof>Science (American Association for the Advancement of Science), 1998-03, Vol.279 (5358), p.1910-1913</ispartof><rights>1998 INIST-CNRS</rights><rights>COPYRIGHT 1998 American Association for the Advancement of Science</rights><rights>COPYRIGHT 1998 American Association for the Advancement of Science</rights><rights>Copyright American Association for the Advancement of Science Mar 20, 1998</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.proquest.com/docview/213554824/fulltextPDF?pq-origsite=primo$$EPDF$$P50$$Gproquest$$H</linktopdf><linktohtml>$$Uhttps://www.proquest.com/docview/213554824?pq-origsite=primo$$EHTML$$P50$$Gproquest$$H</linktohtml><link.rule.ids>314,780,784,21378,21394,27924,27925,33611,33612,33877,33878,43733,43880,74221,74397</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=2241297$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/9506936$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>MCCALL, B. J</creatorcontrib><creatorcontrib>GEBALLE, T. R</creatorcontrib><creatorcontrib>HINKLE, K. H</creatorcontrib><creatorcontrib>OKA, T</creatorcontrib><title>Detection of H3+ in the diffuse interstellar medium toward Cygnus OB2 No. 12</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>The molecular ion H3+ is considered the cornerstone of interstellar chemistry because it initiates the reactions responsible for the production of many larger molecules. Recently discovered in dense molecular clouds, H3+ has now been observed in the diffuse interstellar medium toward Cygnus OB2 No. 12. Analysis of H3+ chemistry suggests that the high H3+ column density (3.8 x 10(14) per square centimeter) is due not to a high H3+ concentration but to a long absorption path. This and other work demonstrate the ubiquity of H3+ and its potential as a probe of the physical and chemical conditions in the interstellar medium.</description><subject>Astronomical Phenomena</subject><subject>Astronomy</subject><subject>Atomic, molecular, chemical, and grain processes</subject><subject>Carbon Monoxide</subject><subject>Cations, Monovalent</subject><subject>Chemistry</subject><subject>Cosmic Dust</subject><subject>Cosmic Radiation</subject><subject>Cygnus (Constellation)</subject><subject>Discovery and exploration</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Extraterrestrial Environment</subject><subject>Interstellar hydrogen</subject><subject>Interstellar medium (ism) and nebulae in milky way</subject><subject>Mathematics</subject><subject>Observations</subject><subject>Organic Chemistry</subject><subject>Space life sciences</subject><subject>Star &amp; galaxy formation</subject><subject>Stellar systems. Galactic and extragalactic objects and systems. The universe</subject><subject>Temperature</subject><subject>Tritium</subject><subject>Vision</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1998</creationdate><recordtype>article</recordtype><sourceid>ALSLI</sourceid><sourceid>CJNVE</sourceid><sourceid>M0P</sourceid><recordid>eNqN0ltrFDEUB_BBlLpWP0IhiKhgZ8x1kjy2q24LS_fBy-uQyZyMKXNpJxlsv30jXYSVRZc8hOT_45DLybITggtCaPkxWA-DhYJKXQgmVEE0wU-yBcFa5Jpi9jRbYMzKXGEpnmcvQrjGOGWaHWVHWuBSs3KRrT9BBBv9OKDRoQv2AfkBxZ-AGu_cHCAtI0whQteZCfXQ-LlHcfxlpgYt79thDmhzTtHVWCBCX2bPnOkCvNrOx9n3L5-_LS_y9WZ1uTxb560gIuacEy3qWpTcKSKl0VqXlsu6JtLi2liliFKqJLJ2daMEcTVvwClsJIVGU8eOs7ePdW-m8XaGEKveB_v7iAOMc6iklpxQxhJ892_IWVkSTcV_S1LClcScJPj6L3g9ztOQrpsME4IryhM6fUSt6aDygxvjZGwLA0ymGwdwPm2fUcyFYiVNPN_D02ig93aff7_jE4lwF1szh1Bdfr06mG5-HEzPV4dStVrv0NN91I5dBy1UqS-Wmx1-sn3euU7dVt1MvjfTfbVt2JS_2eYmWNO5yQzWhz-M0vTxWrIHJtny1w</recordid><startdate>19980320</startdate><enddate>19980320</enddate><creator>MCCALL, B. J</creator><creator>GEBALLE, T. R</creator><creator>HINKLE, K. H</creator><creator>OKA, T</creator><general>American Association for the Advancement of Science</general><general>The American Association for the Advancement of Science</general><scope>IQODW</scope><scope>CGR</scope><scope>CUY</scope><scope>CVF</scope><scope>ECM</scope><scope>EIF</scope><scope>NPM</scope><scope>8GL</scope><scope>IBG</scope><scope>IOV</scope><scope>ISN</scope><scope>0-V</scope><scope>3V.</scope><scope>7QF</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7SS</scope><scope>7T7</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7TM</scope><scope>7U5</scope><scope>7U9</scope><scope>7X2</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88B</scope><scope>88E</scope><scope>88I</scope><scope>8AF</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ALSLI</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>CJNVE</scope><scope>D1I</scope><scope>DWQXO</scope><scope>F28</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>H8G</scope><scope>H94</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9-</scope><scope>K9.</scope><scope>KB.</scope><scope>KR7</scope><scope>L6V</scope><scope>L7M</scope><scope>LK8</scope><scope>L~C</scope><scope>L~D</scope><scope>M0K</scope><scope>M0P</scope><scope>M0R</scope><scope>M0S</scope><scope>M1P</scope><scope>M2O</scope><scope>M2P</scope><scope>M7N</scope><scope>M7P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEDU</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>R05</scope><scope>RC3</scope><scope>7TG</scope><scope>KL.</scope><scope>7X8</scope></search><sort><creationdate>19980320</creationdate><title>Detection of H3+ in the diffuse interstellar medium toward Cygnus OB2 No. 12</title><author>MCCALL, B. J ; GEBALLE, T. R ; HINKLE, K. H ; OKA, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-g515t-44195bb564f8177a9996c47bb17c0bac881888617bfbd851fb4def80a72ed92f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1998</creationdate><topic>Astronomical Phenomena</topic><topic>Astronomy</topic><topic>Atomic, molecular, chemical, and grain processes</topic><topic>Carbon Monoxide</topic><topic>Cations, Monovalent</topic><topic>Chemistry</topic><topic>Cosmic Dust</topic><topic>Cosmic Radiation</topic><topic>Cygnus (Constellation)</topic><topic>Discovery and exploration</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Extraterrestrial Environment</topic><topic>Interstellar hydrogen</topic><topic>Interstellar medium (ism) and nebulae in milky way</topic><topic>Mathematics</topic><topic>Observations</topic><topic>Organic Chemistry</topic><topic>Space life sciences</topic><topic>Star &amp; galaxy formation</topic><topic>Stellar systems. Galactic and extragalactic objects and systems. The universe</topic><topic>Temperature</topic><topic>Tritium</topic><topic>Vision</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>MCCALL, B. J</creatorcontrib><creatorcontrib>GEBALLE, T. R</creatorcontrib><creatorcontrib>HINKLE, K. H</creatorcontrib><creatorcontrib>OKA, T</creatorcontrib><collection>Pascal-Francis</collection><collection>Medline</collection><collection>MEDLINE</collection><collection>MEDLINE (Ovid)</collection><collection>MEDLINE</collection><collection>MEDLINE</collection><collection>PubMed</collection><collection>Gale In Context: High School</collection><collection>Biography resource center</collection><collection>Gale_Opposing Viewpoints In Context</collection><collection>Gale In Context: Canada</collection><collection>ProQuest Social Sciences Premium Collection【Remote access available】</collection><collection>ProQuest Central (Corporate)</collection><collection>Aluminium Industry Abstracts</collection><collection>Animal Behavior Abstracts</collection><collection>Bacteriology Abstracts (Microbiology B)</collection><collection>Calcium &amp; Calcified Tissue Abstracts</collection><collection>Ceramic Abstracts</collection><collection>Chemoreception Abstracts</collection><collection>Computer and Information Systems Abstracts</collection><collection>Corrosion Abstracts</collection><collection>Ecology Abstracts</collection><collection>Electronics &amp; Communications Abstracts</collection><collection>Engineered Materials Abstracts</collection><collection>Entomology Abstracts (Full archive)</collection><collection>Industrial and Applied Microbiology Abstracts (Microbiology A)</collection><collection>Materials Business File</collection><collection>Mechanical &amp; Transportation Engineering Abstracts</collection><collection>Neurosciences Abstracts</collection><collection>Nucleic Acids Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Virology and AIDS Abstracts</collection><collection>Agricultural Science Collection</collection><collection>ProQuest_Health &amp; Medical Collection</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Biology Database (Alumni Edition)</collection><collection>Education Database (Alumni Edition)</collection><collection>Medical Database (Alumni Edition)</collection><collection>Science Database (Alumni Edition)</collection><collection>STEM Database</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Hospital Premium Collection</collection><collection>Hospital Premium Collection (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Social Science Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Advanced Technologies &amp; Aerospace Collection</collection><collection>Agricultural &amp; Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>Biological Science Collection</collection><collection>eLibrary</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Earth, Atmospheric &amp; Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>Education Collection (Proquest) (PQ_SDU_P3)</collection><collection>ProQuest Materials Science Collection</collection><collection>ProQuest Central Korea</collection><collection>ANTE: Abstracts in New Technology &amp; Engineering</collection><collection>Engineering Research Database</collection><collection>Health Research Premium Collection</collection><collection>Health Research Premium Collection (Alumni)</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>Aerospace Database</collection><collection>Copper Technical Reference Library</collection><collection>AIDS and Cancer Research Abstracts</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Materials Research Database</collection><collection>ProQuest Computer Science Collection</collection><collection>Consumer Health Database (Alumni Edition)</collection><collection>ProQuest Health &amp; Medical Complete (Alumni)</collection><collection>Materials Science Database</collection><collection>Civil Engineering Abstracts</collection><collection>ProQuest Engineering Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest Biological Science Collection</collection><collection>Computer and Information Systems Abstracts – Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><collection>Agriculture Science Database</collection><collection>Education Database</collection><collection>ProQuest Family Health</collection><collection>Health &amp; Medical Collection (Alumni Edition)</collection><collection>PML(ProQuest Medical Library)</collection><collection>ProQuest research library</collection><collection>ProQuest Science Journals</collection><collection>Algology Mycology and Protozoology Abstracts (Microbiology C)</collection><collection>ProQuest Biological Science Journals</collection><collection>Engineering Database</collection><collection>Research Library (Corporate)</collection><collection>ProQuest advanced technologies &amp; aerospace journals</collection><collection>ProQuest Advanced Technologies &amp; Aerospace Collection</collection><collection>Biotechnology and BioEngineering Abstracts</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric &amp; Aquatic Science Database</collection><collection>Materials science collection</collection><collection>ProQuest One Education</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><collection>University of Michigan</collection><collection>Genetics Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>MEDLINE - Academic</collection><jtitle>Science (American Association for the Advancement of Science)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>MCCALL, B. J</au><au>GEBALLE, T. R</au><au>HINKLE, K. H</au><au>OKA, T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Detection of H3+ in the diffuse interstellar medium toward Cygnus OB2 No. 12</atitle><jtitle>Science (American Association for the Advancement of Science)</jtitle><addtitle>Science</addtitle><date>1998-03-20</date><risdate>1998</risdate><volume>279</volume><issue>5358</issue><spage>1910</spage><epage>1913</epage><pages>1910-1913</pages><issn>0036-8075</issn><eissn>1095-9203</eissn><coden>SCIEAS</coden><abstract>The molecular ion H3+ is considered the cornerstone of interstellar chemistry because it initiates the reactions responsible for the production of many larger molecules. Recently discovered in dense molecular clouds, H3+ has now been observed in the diffuse interstellar medium toward Cygnus OB2 No. 12. Analysis of H3+ chemistry suggests that the high H3+ column density (3.8 x 10(14) per square centimeter) is due not to a high H3+ concentration but to a long absorption path. This and other work demonstrate the ubiquity of H3+ and its potential as a probe of the physical and chemical conditions in the interstellar medium.</abstract><cop>Washington, DC</cop><pub>American Association for the Advancement of Science</pub><pmid>9506936</pmid><doi>10.1126/science.279.5358.1910</doi><tpages>4</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0036-8075
ispartof Science (American Association for the Advancement of Science), 1998-03, Vol.279 (5358), p.1910-1913
issn 0036-8075
1095-9203
language eng
recordid cdi_proquest_miscellaneous_79741233
source Education Collection (Proquest) (PQ_SDU_P3); JSTOR Archival Journals and Primary Sources Collection; Science Online_科学在线; Social Science Premium Collection (Proquest) (PQ_SDU_P3); Alma/SFX Local Collection
subjects Astronomical Phenomena
Astronomy
Atomic, molecular, chemical, and grain processes
Carbon Monoxide
Cations, Monovalent
Chemistry
Cosmic Dust
Cosmic Radiation
Cygnus (Constellation)
Discovery and exploration
Earth, ocean, space
Exact sciences and technology
Extraterrestrial Environment
Interstellar hydrogen
Interstellar medium (ism) and nebulae in milky way
Mathematics
Observations
Organic Chemistry
Space life sciences
Star & galaxy formation
Stellar systems. Galactic and extragalactic objects and systems. The universe
Temperature
Tritium
Vision
title Detection of H3+ in the diffuse interstellar medium toward Cygnus OB2 No. 12
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-26T04%3A17%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-gale_proqu&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Detection%20of%20H3+%20in%20the%20diffuse%20interstellar%20medium%20toward%20Cygnus%20OB2%20No.%2012&rft.jtitle=Science%20(American%20Association%20for%20the%20Advancement%20of%20Science)&rft.au=MCCALL,%20B.%20J&rft.date=1998-03-20&rft.volume=279&rft.issue=5358&rft.spage=1910&rft.epage=1913&rft.pages=1910-1913&rft.issn=0036-8075&rft.eissn=1095-9203&rft.coden=SCIEAS&rft_id=info:doi/10.1126/science.279.5358.1910&rft_dat=%3Cgale_proqu%3EA20458362%3C/gale_proqu%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-g515t-44195bb564f8177a9996c47bb17c0bac881888617bfbd851fb4def80a72ed92f3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=213554824&rft_id=info:pmid/9506936&rft_galeid=A20458362&rfr_iscdi=true