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dc.date.accessioned 2020-06-22T13:22:58Z
dc.date.available 2020-06-22T13:22:58Z
dc.date.issued 1973
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/98701
dc.description.abstract van Rhijn’s method is used to derive the luminosity function in the solar neighbourhood from large proper motion stars. The values obtained are smaller than the currently accepted ones; for M_B < 9, the factor is of the order of two. It is shown that these differences arise from the systematic errors of other methods, specially for non-inclusion of the correction for the errors of the parallaxes. The luminosity function has some irregularities, not previously found because of smoothing. A secondary maximum near M_B = 11 , particularly, seems to be a real feature. en
dc.language es es
dc.subject Galaxias es
dc.title The luminosity function in the solar neighbourhood en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Muzzio, J.C. 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. 17 es


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