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HI Absorption in a Gravitational Lens at z ~ 0.7645

Kanekar, N; Briggs, Franklin

Description

We have used the Westerbork Synthesis Radio Telescope to detect HI 21 cm absorption at z ∼ 0.7645 in the gravitational lens system towards PMN J0134-0931. The 21 cm profile has two broad components, with peak optical depths of 0.047 ± 0.007 and 0.039 �

dc.contributor.authorKanekar, N
dc.contributor.authorBriggs, Franklin
dc.date.accessioned2015-12-13T23:09:37Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/87078
dc.description.abstractWe have used the Westerbork Synthesis Radio Telescope to detect HI 21 cm absorption at z ∼ 0.7645 in the gravitational lens system towards PMN J0134-0931. The 21 cm profile has two broad components, with peak optical depths of 0.047 ± 0.007 and 0.039 �
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Galaxies; Gravitation; Mathematical models; Radio telescopes; Space research; Gravitational lensing; Lensing galaxy; Astrophysics 0931; Galaxies: Individual: PMN J0134; Gravitational lensing; ISM; Radio lines
dc.titleHI Absorption in a Gravitational Lens at z ~ 0.7645
dc.typeJournal article
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.citationvolume412
dc.date.issued2003
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub16214
local.type.statusPublished Version
local.contributor.affiliationKanekar, N, National Radio Astronomy Observatory
local.contributor.affiliationBriggs, Franklin, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.startpageL29
local.bibliographicCitation.lastpageL32
local.identifier.doi10.1051/0004-6361:20031676
dc.date.updated2015-12-12T08:19:57Z
local.identifier.scopusID2-s2.0-0346885683
CollectionsANU Research Publications

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