HST /COS DETECTION OF DEUTERATED MOLECULAR HYDROGEN IN A DAMPED Lyα SYSTEM AT z = 0.18
We report on the detection of deuterated molecular hydrogen, HD, at z = 0.18. HD and H sub(2) are detected in HST/COS data of a low-metallicity (Z ~ 0.07 Z sub([middot in circle])) damped Ly alpha (DLA) system at z = 0.18562 toward QSO B0120-28, with log N(H I) = 20.50 + or - 0.10. Four absorption c...
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description | We report on the detection of deuterated molecular hydrogen, HD, at z = 0.18. HD and H sub(2) are detected in HST/COS data of a low-metallicity (Z ~ 0.07 Z sub([middot in circle])) damped Ly alpha (DLA) system at z = 0.18562 toward QSO B0120-28, with log N(H I) = 20.50 + or - 0.10. Four absorption components are clearly resolved in H sub(2), while two components are resolved in HD; the bulk of the molecular hydrogen is associated with the components traced by HD. We find total column densities log N(HD) = 14.82 + or - 0.15 and log N(H sub(2)) = 20.00 + or - 0.10. This system has a high molecular fraction, f(H sub(2)) = 0.39 + or - 0.10, and a low HD-to-H sub(2) ratio, log (HD/2H sub(2)) = -5.5 + or - 0.2 dex. The excitation temperature, T sub(01) = 65 + or - 2 K, in the component containing the bulk of the molecular gas is lower than in other DLAs. These properties are unlike those in other higher redshift DLA systems known to contain HD, but are consistent with what is observed in dense clouds in the Milky Way. |
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HD and H sub(2) are detected in HST/COS data of a low-metallicity (Z ~ 0.07 Z sub([middot in circle])) damped Ly alpha (DLA) system at z = 0.18562 toward QSO B0120-28, with log N(H I) = 20.50 + or - 0.10. Four absorption components are clearly resolved in H sub(2), while two components are resolved in HD; the bulk of the molecular hydrogen is associated with the components traced by HD. We find total column densities log N(HD) = 14.82 + or - 0.15 and log N(H sub(2)) = 20.00 + or - 0.10. This system has a high molecular fraction, f(H sub(2)) = 0.39 + or - 0.10, and a low HD-to-H sub(2) ratio, log (HD/2H sub(2)) = -5.5 + or - 0.2 dex. The excitation temperature, T sub(01) = 65 + or - 2 K, in the component containing the bulk of the molecular gas is lower than in other DLAs. These properties are unlike those in other higher redshift DLA systems known to contain HD, but are consistent with what is observed in dense clouds in the Milky Way.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/783/1/22</identifier><language>eng</language><publisher>United States</publisher><subject>ABSORPTION ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Bulk density ; Clouds ; Density ; DETECTION ; Deuteration ; EXCITATION ; GAMMA-GAMMA LOGGING ; HYDROGEN ; Hydrogen storage ; METALLICITY ; MILKY WAY ; MOLECULES ; QUASARS ; RED SHIFT</subject><ispartof>The Astrophysical journal, 2014-03, Vol.783 (1), p.1-7, Article 22</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c341t-bdd4d9cf846d91c2597737e44ce28e9e1622e4c9db673f1df7fb87a7ab1abefa3</citedby><cites>FETCH-LOGICAL-c341t-bdd4d9cf846d91c2597737e44ce28e9e1622e4c9db673f1df7fb87a7ab1abefa3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,778,782,883,27911,27912</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22351385$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Oliveira, Cristina M</creatorcontrib><creatorcontrib>SEMBACH, KENNETH R</creatorcontrib><creatorcontrib>Tumlinson, Jason</creatorcontrib><creatorcontrib>O'Meara, John</creatorcontrib><creatorcontrib>Thom, Christopher</creatorcontrib><title>HST /COS DETECTION OF DEUTERATED MOLECULAR HYDROGEN IN A DAMPED Lyα SYSTEM AT z = 0.18</title><title>The Astrophysical journal</title><description>We report on the detection of deuterated molecular hydrogen, HD, at z = 0.18. HD and H sub(2) are detected in HST/COS data of a low-metallicity (Z ~ 0.07 Z sub([middot in circle])) damped Ly alpha (DLA) system at z = 0.18562 toward QSO B0120-28, with log N(H I) = 20.50 + or - 0.10. Four absorption components are clearly resolved in H sub(2), while two components are resolved in HD; the bulk of the molecular hydrogen is associated with the components traced by HD. We find total column densities log N(HD) = 14.82 + or - 0.15 and log N(H sub(2)) = 20.00 + or - 0.10. This system has a high molecular fraction, f(H sub(2)) = 0.39 + or - 0.10, and a low HD-to-H sub(2) ratio, log (HD/2H sub(2)) = -5.5 + or - 0.2 dex. The excitation temperature, T sub(01) = 65 + or - 2 K, in the component containing the bulk of the molecular gas is lower than in other DLAs. These properties are unlike those in other higher redshift DLA systems known to contain HD, but are consistent with what is observed in dense clouds in the Milky Way.</description><subject>ABSORPTION</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Bulk density</subject><subject>Clouds</subject><subject>Density</subject><subject>DETECTION</subject><subject>Deuteration</subject><subject>EXCITATION</subject><subject>GAMMA-GAMMA LOGGING</subject><subject>HYDROGEN</subject><subject>Hydrogen storage</subject><subject>METALLICITY</subject><subject>MILKY WAY</subject><subject>MOLECULES</subject><subject>QUASARS</subject><subject>RED SHIFT</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><recordid>eNqNkc1Og0AUhSdGE2v1BVxN4sYNwvzQGRYuCKU_CS2mpdGuJsMwRAwFZeiivpUv4jMJqXHhwri6ObnfvffkHgCukXOHHM5tx3GoNSLsyWac2MjG-AQMkEu4RYnLTsHgBzgHF8a89BJ73gA8ztYJtIN4DcdhEgbJPF7CeNKJTRKu_CQcw0UchcEm8ldwth2v4mm4hPMl9OHYXzx07ejw-QHX23USLqCfwHd4DztP_BKc5bI0-uq7DsFmEibBzIri6TzwI0sRilorzTKaeSrndJR5SGHXY4wwTanSmGtPoxHGmiovS0eM5CjLWZ5yJplMkUx1LskQ3Bz31qYthFFFq9WzqqtKq1ZgTFxEuNtRt0fqtanf9tq0YlcYpctSVrreG4GY0x1mlDr_QRHlCGHWofiIqqY2ptG5eG2KnWwOAjmij0X0bxb910UXi0C9oSHgv4Y6z7It6qptZFH-NfoFbfOJ5A</recordid><startdate>20140301</startdate><enddate>20140301</enddate><creator>Oliveira, Cristina M</creator><creator>SEMBACH, KENNETH R</creator><creator>Tumlinson, Jason</creator><creator>O'Meara, John</creator><creator>Thom, Christopher</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20140301</creationdate><title>HST /COS DETECTION OF DEUTERATED MOLECULAR HYDROGEN IN A DAMPED Lyα SYSTEM AT z = 0.18</title><author>Oliveira, Cristina M ; SEMBACH, KENNETH R ; Tumlinson, Jason ; O'Meara, John ; Thom, Christopher</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c341t-bdd4d9cf846d91c2597737e44ce28e9e1622e4c9db673f1df7fb87a7ab1abefa3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>ABSORPTION</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Bulk density</topic><topic>Clouds</topic><topic>Density</topic><topic>DETECTION</topic><topic>Deuteration</topic><topic>EXCITATION</topic><topic>GAMMA-GAMMA LOGGING</topic><topic>HYDROGEN</topic><topic>Hydrogen storage</topic><topic>METALLICITY</topic><topic>MILKY WAY</topic><topic>MOLECULES</topic><topic>QUASARS</topic><topic>RED SHIFT</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Oliveira, Cristina M</creatorcontrib><creatorcontrib>SEMBACH, KENNETH R</creatorcontrib><creatorcontrib>Tumlinson, Jason</creatorcontrib><creatorcontrib>O'Meara, John</creatorcontrib><creatorcontrib>Thom, Christopher</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Oliveira, Cristina M</au><au>SEMBACH, KENNETH R</au><au>Tumlinson, Jason</au><au>O'Meara, John</au><au>Thom, Christopher</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>HST /COS DETECTION OF DEUTERATED MOLECULAR HYDROGEN IN A DAMPED Lyα SYSTEM AT z = 0.18</atitle><jtitle>The Astrophysical journal</jtitle><date>2014-03-01</date><risdate>2014</risdate><volume>783</volume><issue>1</issue><spage>1</spage><epage>7</epage><pages>1-7</pages><artnum>22</artnum><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>We report on the detection of deuterated molecular hydrogen, HD, at z = 0.18. HD and H sub(2) are detected in HST/COS data of a low-metallicity (Z ~ 0.07 Z sub([middot in circle])) damped Ly alpha (DLA) system at z = 0.18562 toward QSO B0120-28, with log N(H I) = 20.50 + or - 0.10. Four absorption components are clearly resolved in H sub(2), while two components are resolved in HD; the bulk of the molecular hydrogen is associated with the components traced by HD. We find total column densities log N(HD) = 14.82 + or - 0.15 and log N(H sub(2)) = 20.00 + or - 0.10. This system has a high molecular fraction, f(H sub(2)) = 0.39 + or - 0.10, and a low HD-to-H sub(2) ratio, log (HD/2H sub(2)) = -5.5 + or - 0.2 dex. The excitation temperature, T sub(01) = 65 + or - 2 K, in the component containing the bulk of the molecular gas is lower than in other DLAs. These properties are unlike those in other higher redshift DLA systems known to contain HD, but are consistent with what is observed in dense clouds in the Milky Way.</abstract><cop>United States</cop><doi>10.1088/0004-637X/783/1/22</doi><tpages>7</tpages></addata></record> |
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subjects | ABSORPTION ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Bulk density Clouds Density DETECTION Deuteration EXCITATION GAMMA-GAMMA LOGGING HYDROGEN Hydrogen storage METALLICITY MILKY WAY MOLECULES QUASARS RED SHIFT |
title | HST /COS DETECTION OF DEUTERATED MOLECULAR HYDROGEN IN A DAMPED Lyα SYSTEM AT z = 0.18 |
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