Please use this identifier to cite or link to this item:
https://dspace.ffh.bg.ac.rs/handle/123456789/1265
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ignjatović, Ljubiša | en |
dc.contributor.author | Mihajlov, A. A. | en |
dc.contributor.author | Metropoulos, A. | en |
dc.contributor.author | Sakan, N. M. | en |
dc.contributor.author | Dimitrijević, M. S. | en |
dc.date.accessioned | 2022-12-16T17:49:50Z | - |
dc.date.available | 2022-12-16T17:49:50Z | - |
dc.date.issued | 2010-02-22 | en |
dc.identifier.isbn | 9780735407404 | en |
dc.identifier.issn | 0094-243X | en |
dc.identifier.uri | https://dspace.ffh.bg.ac.rs/handle/123456789/1265 | - |
dc.description.abstract | The 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.ispartof | AIP Conference Proceedings | en |
dc.subject | Atmospheres | en |
dc.subject | Atomic processes | en |
dc.subject | Molecular processes | en |
dc.subject | Radiative transfer | en |
dc.title | The contribution of the absorption processes to the opacity of DB white dwarf atmospheres in UV and VUV regions | en |
dc.type | Conference Paper | en |
dc.identifier.doi | 10.1063/1.3322343 | en |
dc.identifier.scopus | 2-s2.0-76749085797 | en |
dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/76749085797 | en |
dc.relation.firstpage | 121 | en |
dc.relation.lastpage | 126 | en |
dc.relation.volume | 1203 | en |
item.grantfulltext | none | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference Paper | - |
item.fulltext | No Fulltext | - |
item.cerifentitytype | Publications | - |
Appears in Collections: | Journal Article |
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