The high-redshift deuterium abundance: The z = 3.086 absorption complex towards Q 0420 - 388

Monthly Notices of the Royal Astronomical Society

Volumn 278, Issue 2, 1996, Pages 506-518

  Carswell, R F ^a   Webb, J K ^b   Lanzetta, K M ^c   Baldwin, J A ^d   Cooke, A J ^d,e   Williger, G M ^d,f   Rauch, M ^g   Irwin, M J ^h   Robertson, J G ⁱ   Shaver, P A ^j  

^a UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^b UNIVERSITY OF NEW SOUTH WALES   (Australia)

^c STONY BROOK UNIVERSITY   (United States)

^d CERRO TOLOLO INTER AMERICAN OBSERVATORY   (Chile)

^e UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^f MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^g CARNEGIE OBSERVATORIES   (United States)

^h ROYAL GREENWICH OBSERVATORY   (United Kingdom)

ⁱ UNIVERSITY OF SYDNEY   (Australia)

^j EUROPEAN SOUTHERN OBSERVATORY   (Germany)

more..

Author keywords

Galaxies: abundances; Quasars: absorption lines; Quasars: individual: 0420 388

Indexed keywords

COSMOLOGY; GALAXIES;

COLUMN DENSITY; ELEMENT ABUNDANCES; GALAXIES ABUNDANCES; HEAVY ELEMENTS; HIGH-ORDER; HIGH-REDSHIFT; QUASAR: INDIVIDUAL: 0420-388; QUASARS ABSORPTION LINES; QUASARS: INDIVIDUAL;

DEUTERIUM;

EID: 0001395911     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/278.2.506     Document Type: Article

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