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Please use this identifier to cite or link to this item: https://dspace.ffh.bg.ac.rs/handle/123456789/1265
DC FieldValueLanguage
dc.contributor.authorIgnjatović, Ljubišaen
dc.contributor.authorMihajlov, A. A.en
dc.contributor.authorMetropoulos, A.en
dc.contributor.authorSakan, N. M.en
dc.contributor.authorDimitrijević, M. S.en
dc.date.accessioned2022-12-16T17:49:50Z-
dc.date.available2022-12-16T17:49:50Z-
dc.date.issued2010-02-22en
dc.identifier.isbn9780735407404en
dc.identifier.issn0094-243Xen
dc.identifier.urihttps://dspace.ffh.bg.ac.rs/handle/123456789/1265-
dc.description.abstractThe main aim of this work is to estimate the total contribution to the opacity of DB white dwarf atmosphere of the processes of the He2+ molecular ion photo-dissociation and He + He+ collisional absorption charge exchange, and compare it with the contribution of He-, and other relevant, radiative absorption processes included in standard models. © 2009 American Institute of Physics.en
dc.relation.ispartofAIP Conference Proceedingsen
dc.subjectAtmospheresen
dc.subjectAtomic processesen
dc.subjectMolecular processesen
dc.subjectRadiative transferen
dc.titleThe contribution of the absorption processes to the opacity of DB white dwarf atmospheres in UV and VUV regionsen
dc.typeConference Paperen
dc.identifier.doi10.1063/1.3322343en
dc.identifier.scopus2-s2.0-76749085797en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/76749085797en
dc.relation.firstpage121en
dc.relation.lastpage126en
dc.relation.volume1203en
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairetypeConference Paper-
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University of Belgrade
Faculty of Physical Chemistry
Studentski trg 12-16
11158 Belgrade 118
PAC 105305
SERBIA
University of Belgrade Faculty of Physical Chemistry