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dc.date.accessioned 2022-09-01T15:37:08Z
dc.date.available 2022-09-01T15:37:08Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/141449
dc.description.abstract The absolute proper motion of the primary component of this pair is derived on the basis of all available photographic and meridian observations, spanning over 55 years. The relative trajectory is then computed from all existing differential measurements, and different criteria were used to show that the pair is optical. An ephemeris is presented for the interval 1988-2000. The proper motion for the secondary component is obtained by combining that of the primary with the relative motion, achieving a much higher precision than that allowed by the very few absolute observations of the secondary alone. Both proper motions are finally compared with other determinations. The complete version of this work will be published elsewhere. en
dc.language es es
dc.subject Galaxia es
dc.title Analysis of the absolute and relative astrometric observation of the visual double star HJ 3370 AC en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Torres, G. 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. 33 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)