APROXIMACION GEOMÉTRICA DEL POLO NORTE GALÁCTICO MEDIANTE ESTRELLAS DEL DISCO GALÁCTICO

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dc.contributor.authorLUDVING CANO
dc.coverage.spatialBolivia
dc.date.accessioned2026-03-22T18:58:30Z
dc.date.available2026-03-22T18:58:30Z
dc.date.issued2022
dc.description.abstractWe present a geometrical method to estimate the equatorial coordinates of the North Galactic Pole, using stars from the Milky Way disk. First we explain the method used and then, with 4 astronomical catalogs, we obtain the coordinates. We found that the results are not very accurate but are pretty close. This is mostly because the catalogs have extreme points or stars that are not uniformly distributed in the galactic disk.
dc.identifier.doi10.53287/upvs6575hp32y
dc.identifier.urihttps://doi.org/10.53287/upvs6575hp32y
dc.identifier.urihttps://andeanlibrary.org/handle/123456789/73306
dc.language.isoen
dc.relation.ispartofRevista Boliviana de Física
dc.sourceHigher University of San Andrés
dc.subjectMilky Way
dc.subjectStars
dc.subjectPhysics
dc.subjectDisc
dc.subjectAstrophysics
dc.subjectAstronomy
dc.titleAPROXIMACION GEOMÉTRICA DEL POLO NORTE GALÁCTICO MEDIANTE ESTRELLAS DEL DISCO GALÁCTICO
dc.typearticle

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