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LAReferencia - Red Federada de Repositorios Institucionales de Publicaciones Científicas Latinoamericanas
Doctoral thesis . 2008
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Propiedades físicas de estrellas con exoplanetas y anillos circunestelares

descriptionPublicationkeyboard_double_arrow_right Doctoral thesis 01 Mar 2008 Argentina Spanish; Castilian
Authors: Saffe Jameson, Carlos Emilio;

handle: 11086/122

Propiedades físicas de estrellas con exoplanetas y anillos circunestelares

Abstract

Estudiamos diferentes aspectos de estrellas con exoplanetas (EH) y de estrellas de tipo Vega. Detectamos excesos IR en 20% de las estrellas EH, el cual se atribuye a la presencia de polvo circunestelar.

Tesis (Doctor en Astronomía)--Universidad Nacional de Córdoba. Facultad de Matemática, Astronomía y Física, 2008.

Country
Argentina
Related Organizations
Keywords

Excesos infrarrojos, Sistemas planetarios extrasolares, Abundances, chemical composition, Metalicidad, Extrasolar planetary systems, Planetas, chemical composition, Abundances, Stellar atmospheres, Estrellas con discos de polvo

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    popularity
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    		 Average
    influence
    This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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    impulse
    This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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Powered by OpenAIRE graph
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Green