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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/2882
DC FieldValueLanguage
dc.contributor.authorOnić, Dušanen_US
dc.contributor.authorČadež, Vladimiren_US
dc.date.accessioned2025-11-05T09:50:27Z-
dc.date.available2025-11-05T09:50:27Z-
dc.date.issued2010-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/2882-
dc.description.abstractThe effect of black body radiation on convective stability in stellar plasmas is twofold. It enters analytical expressions for adiabatic processes and for plasma density distribution in hydrostatic equilibrium. We derive and analyze the condition for onset of convective instability assuming small adiabatic displacements of fluid particles in stratified plasma with prescribed model temperature profiles.en_US
dc.language.isoenen_US
dc.publisherBeograd : Astronomska opservatorijaen_US
dc.relation.ispartofPublications of the Astronomical Observatory of Belgradeen_US
dc.titleEffects Of Radiation On Convective Instability In Stratified Stellar Plasmasen_US
dc.typeConference Objecten_US
dc.relation.conferenceSommer School and International Symposium on Physics of Ionized Gases (24 ; 2010 ; Donji Milanovac)en_US
dc.relation.publication24th Summer school and international symposium on the physics of ionized gasesen_US
dc.identifier.urlhttps://publications.aob.rs/89/pdf/379-382.pdf-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0373-3742en_US
dc.description.rankM33en_US
dc.relation.firstpage379en_US
dc.relation.lastpage382en_US
dc.relation.volume89en_US
item.openairetypeConference Object-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-2130-2011-
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