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dc.date.accessioned 2022-06-27T13:03:35Z
dc.date.available 2022-06-27T13:03:35Z
dc.date.issued 1987
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/138373
dc.description.abstract Surface photographic photometry was not extended to low enough levels in order to warrant a suitable extrapolation leading to total magnitudes. We have computed, consequently, the luminosity up to the last measured isophote and we have obtained two parameters from the IS curve. Then, the values of N and Qₙ follow from double interpolation in a family of curves for integer values of N. Since Qₙ is known, we obtain the total luminosity Lₜ=QₙIₙSₙ and the total magnitude for each galaxy. en
dc.language es es
dc.subject Galaxias es
dc.title Calculation of total magnitude of galaxies en
dc.type Articulo es
sedici.identifier.issn 1669-9521 es
sedici.creator.person Alonso, María Victoria es
sedici.creator.person Sérsic, José Luis 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)