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dc.date.accessioned 2019-04-24T12:50:45Z
dc.date.available 2019-04-24T12:50:45Z
dc.date.issued 1960
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/74443
dc.description.abstract In current literature on degenerated stellar configurations there seems to exist a strange misconception concerning the equations for relativistic degeneracv. As it is well known in a non-relativistic degenerated gas we can neglect the partial pressure of heavy particles due to the fact that in the equation of state for non-relativistic degeneracy the mass of the particles is contained in the denominator: with the usual notation. en
dc.language es es
dc.subject degenerated stellar configurations es
dc.subject Galaxias es
dc.title A comment on the equation of state for a degenerated gas en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Gratton, Livio es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Asociación Argentina de Astronomía es
sedici.subtype Comunicacion es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 2 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)