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dc.date.accessioned | 2020-06-19T12:20:46Z | |
dc.date.available | 2020-06-19T12:20:46Z | |
dc.date.issued | 1971 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/98560 | |
dc.description.abstract | These stellar recounts averaged over all galactic latitudes are analysed by a series of Kapteyn-schemes. In this way, “artificial” stellar count without and with general interstellar absorption are originated. All these curves can be represented, almost until m=20, by one unique interpolation formula, function of the galactic latitude and of the apparent magnitude. | en |
dc.language | es | es |
dc.subject | Galaxias | es |
dc.title | Una nueva interpretación de los recuentos estelares promedios de Seares, van Rhijn, Joyner y Richmond 1925 Ap.J. 62 | es |
dc.type | Articulo | es |
sedici.identifier.issn | 1669-9521 | es |
sedici.creator.person | Wilkens, Herbert | 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. 16 | es |