Show simple item record

dc.contributor.authorMelis, Carl
dc.contributor.authorDufour, P.
dc.contributor.authorFarihi, J.
dc.contributor.authorBochanski, John J.
dc.contributor.authorBurgasser, Adam J.
dc.contributor.authorParsons, S. G.
dc.contributor.authorGansicke, Boris T.
dc.contributor.authorKoester, D.
dc.contributor.authorSwift, Brandon J.
dc.date.accessioned2015-02-27T15:01:03Z
dc.date.available2015-02-27T15:01:03Z
dc.date.issued2012-05
dc.date.submitted2012-03
dc.identifier.issn2041-8205
dc.identifier.issn2041-8213
dc.identifier.urihttp://hdl.handle.net/1721.1/95716
dc.description.abstractWe present new spectroscopic observations of the polluted, dusty, helium-dominated atmosphere white dwarf star HE 1349–2305. Optical spectroscopy reveals weak Ca II infrared triplet emission indicating that metallic gas debris orbits and is accreted by the white dwarf. Atmospheric abundances are measured for magnesium and silicon while upper limits for iron and oxygen are derived from the available optical spectroscopy. HE 1349–2305 is the first gas disk-hosting white dwarf star identified among previously known polluted white dwarfs. Further characterization of the parent body polluting this star will require ultraviolet spectroscopy.en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (Award No. AST-1003318)en_US
dc.description.sponsorshipCentre de recherche en astrophysique du Québec (CRAQ postdoctoral fellow)en_US
dc.description.sponsorshipNatural Sciences and Engineering Research Council Canadaen_US
dc.description.sponsorshipFonds québécois de la recherche sur la nature et les technologies (Fund FQRNT Québec)en_US
dc.language.isoen_US
dc.publisherInstitute of Physics/American Astronomical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1088/2041-8205/751/1/l4en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Astronomical Societyen_US
dc.titleGASEOUS MATERIAL ORBITING THE POLLUTED, DUSTY WHITE DWARF HE 1349–2305en_US
dc.typeArticleen_US
dc.identifier.citationMelis, Carl, P. Dufour, J. Farihi, J. Bochanski, Adam J. Burgasser, S. G. Parsons, B. T. Gansicke, D. Koester, and Brandon J. Swift. “GASEOUS MATERIAL ORBITING THE POLLUTED, DUSTY WHITE DWARF HE 1349–2305.” The Astrophysical Journal 751, no. 1 (April 30, 2012): L4. © 2012 American Astronomical Society.en_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorBurgasser, Adam J.en_US
dc.relation.journalAstrophysical Journalen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsMelis, Carl; Dufour, P.; Farihi, J.; Bochanski, J.; Burgasser, Adam J.; Parsons, S. G.; Gänsicke, B. T.; Koester, D.; Swift, Brandon J.en_US
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record