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dc.date.accessioned 2022-10-04T14:16:02Z
dc.date.available 2022-10-04T14:16:02Z
dc.date.issued 1990
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/143257
dc.description.abstract We have studied the spectrum of the star HD 37129 which is a member of the Orion OB1 association. We have found that the helium abundance is normal and some iron peak elements are enhanced as well as manganese, phosphorus and mercury. The adopted effective temperature is 18750 K. We have compared the spectrum with a standard star, ι Her, and a "sn" peculiar star. We conclude that HD 37129 is a "sn" peculiar star with helium normal. en
dc.language es es
dc.subject Galaxia es
dc.title Is HD 37129 a peculiar star? en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Malaroda, Stella Maris es
sedici.creator.person Pintado, O.I. 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. 36 es
dc.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)


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