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dc.date.accessioned 2022-09-22T14:22:49Z
dc.date.available 2022-09-22T14:22:49Z
dc.date.issued 1988
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/142563
dc.description.abstract We have studied, in the photographic and UV regions, stars presenting forbidden components of He I in absorption. With the aid of theoretical models available in the literature, we have concluded that dissipation of mechanical energy is more important in equatorial regions. We have also observed that ionized Fe and Mg present higher expansion velocities at the polar regions. en
dc.language es es
dc.subject Galaxia es
dc.title Relations between He I and circumstellar Fe II and Mg II en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Ringuelet, Adela Emilia es
sedici.creator.person es
sedici.subject.materias Astronomía 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. 34 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)