H I 21 cm Observations of the PG 1216+069 Sub-Damped Lγα Absorber Field at z = 0.00632

dc.contributor.authorBriggs, Franklin
dc.contributor.authorBarnes, David G
dc.date.accessioned2015-12-07T22:30:57Z
dc.date.issued2006
dc.date.updated2015-12-07T10:10:48Z
dc.description.abstractThe Westerbork Synthesis Radio Telescope finds a weak 21 cm line emission feature at the coordinates (R.A., decl., velocity) of the sub-damped Lyα (DLA) absorber observed at zabs = 0.00632 in the spectrum of PG 1216+069. The emission feature, WSRT J12192
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/22557
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Cosmology: observations; Galaxies: formation; Galaxies: individual (VCC 297, VCC 327, VCC 339); Intergalactic medium; Quasars: absorption lines; Quasars: individual (PG 1216+069); Radio lines: galaxies
dc.titleH I 21 cm Observations of the PG 1216+069 Sub-Damped Lγα Absorber Field at z = 0.00632
dc.typeJournal article
local.bibliographicCitation.lastpageL130
local.bibliographicCitation.startpageL127
local.contributor.affiliationBriggs, Franklin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBarnes, David G, University of Melbourne
local.contributor.authoremailu4049161@anu.edu.au
local.contributor.authoruidBriggs, Franklin, u4049161
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4370312xPUB22
local.identifier.citationvolume640
local.identifier.doi10.1086/503525
local.identifier.scopusID2-s2.0-33645824532
local.identifier.uidSubmittedByu4370312
local.type.statusPublished Version

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