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dc.date.accessioned 2020-03-25T11:00:56Z
dc.date.available 2020-03-25T11:00:56Z
dc.date.issued 1963
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/91598
dc.description.abstract On the basis of Coudé material generously loaned by Dr. H. Babcook, about 250 lines were measured in the wavelength region λ ∼ 3800 - 4600. A 94 % of them were identified. Of this percentage, 40 % belong to Mn II. In both stars C II is too strong for this type. P II was not detected. Y II is surprisingly strong, with a slight difference in the enhancement between both stars. The stars were also compared with two other manganese stars already analysed at high dispersion. The full paper will be published somewhere else. en
dc.format.extent 31-31 es
dc.language en es
dc.subject espectroscopía es
dc.subject Estrellas es
dc.title A spectroscopic study of the peculiar stars μ Lep and χ Boo en
dc.type Articulo es
sedici.creator.person Jaschek, Mercedes es
sedici.creator.person Jaschek, Carlos 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.event VI Reunión Científica de la Asociación Argentina de Astronomía (Horco Molle, Tucumán, 22 al 25 de mayo de 1963) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Boletín de la Asociación Argentina de Astronomía es
sedici.relation.journalVolumeAndIssue no. 6 es
dc.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/ es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)