The richest globular clusters in variable stars

dc.creatorWilkens, Herbert
dc.date1963
dc.date2020-03-17T12:35:50Z
dc.date.accessioned2023-07-14T18:59:32Z
dc.date.available2023-07-14T18:59:32Z
dc.identifierhttp://sedici.unlp.edu.ar/handle/10915/90963
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7433571
dc.descriptionThe publication of the figures of 37 globular clusters (only 2 figures in this Bulletin) characterized by possessing variable stars in them - while the variables of the surrounding field appear more or less separated from them - has the object of proving that the apparent diameter of these clusters were estimated correctly with the help of these variables. These apparent diameters were the base of a previous theoretical investigation of the author on "Luminosity and diameter of globular clusters I", La Plata, Serie Circular Nº 16. The paper will be published in the same "serie Circular".
dc.descriptionAsociación Argentina de Astronomía
dc.formatapplication/pdf
dc.languagees
dc.rightshttp://creativecommons.org/licenses/by-nc-sa/4.0/
dc.rightsCreative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.subjectCiencias Astronómicas
dc.subjectCúmulos globulares
dc.subjectdiiámetros
dc.titleLos cúmulos globulares más ricos en estrellas variables
dc.titleThe richest globular clusters in variable stars
dc.typeArticulo
dc.typeArticulo


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