Carbon and Hydrogen in Hot DB White Dwarfs

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dc.contributor.authorProvencal, J
dc.contributor.authorShipman, H
dc.contributor.authorThejll, P
dc.contributor.authorVennes, Stephane
dc.date.accessioned2015-12-13T23:16:06Z
dc.date.issued2000
dc.date.updated2015-12-12T08:46:38Z
dc.description.abstractThe roles played by carbon and hydrogen in helium atmosphere (DB) white dwarf evolution is not well understood. We present GHRS observations (centered at 1215 and 1335 Å) of the hot helium white dwarfs PG 0112+104 (≈30,000 K) and GD 190 (≈23,000 K) a
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/89237
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Stars: individual (GD 190, GD 358, PG 0112+104); Ultraviolet: stars; White dwarfs
dc.titleCarbon and Hydrogen in Hot DB White Dwarfs
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage1056
local.bibliographicCitation.startpage1041
local.contributor.affiliationProvencal, J, University of Delaware
local.contributor.affiliationShipman, H, University of Delaware
local.contributor.affiliationThejll, P, Danish Meteorological Institute
local.contributor.affiliationVennes, Stephane, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidVennes, Stephane, u9711096
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub19201
local.identifier.citationvolume542
local.identifier.scopusID2-s2.0-0034692702
local.type.statusPublished Version

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