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dc.contributor.authorWatson, D.
dc.contributor.authorHjorth, J.
dc.contributor.authorFynbo, J.
dc.contributor.authorJakobsson, P.
dc.contributor.authorFoley, S.
dc.contributor.authorSollerman, J.
dc.contributor.authorWijers, R.A.M.J.
dc.date.accessioned2009-01-06T11:55:57Z
dc.date.available2009-01-06T11:55:57Z
dc.date.issued2007
dc.identifier.citationWatson , D , Hjorth , J , Fynbo , J , Jakobsson , P , Foley , S , Sollerman , J & Wijers , R A M J 2007 , ' Very different X-ray to optical column density ratios in gamma-ray burst afterglows: ionisation in GRB environments ' , The Astrophysical Journal , vol. 660 , no. 2 , L101 . https://doi.org/10.1086/518310
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 151642
dc.identifier.otherPURE UUID: 8ed481a7-c212-4911-bee4-fb823eed4617
dc.identifier.otherdspace: 2299/2749
dc.identifier.otherScopus: 34249899945
dc.identifier.urihttp://hdl.handle.net/2299/2749
dc.descriptionOriginal article can be found at: http://www.iop.org/EJ/journal/apjl Copyright American Astronomical Society DOI: 10.1086/518310 [Full text of this article is not available in the UHRA]
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleVery different X-ray to optical column density ratios in gamma-ray burst afterglows: ionisation in GRB environmentsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.versionofrecordhttps://doi.org/10.1086/518310
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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