On galactic absorption

dc.creatorTovmassian Hrant
dc.creatorMonica Rodriguez
dc.date2008
dc.date.accessioned2023-07-25T16:22:55Z
dc.date.available2023-07-25T16:22:55Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1070
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7806270
dc.descriptionWe show that the stellar photored magnitude, m₁₀, of the 10th by brightness galaxy in an Abell cluster is not a good indicator of the cluster distance. We find that the values of m₁₀ for clusters in the southern Galactic hemisphereare systematically fainter by about 0 ͫ. 17 than those in the northern hemisphere. This may be due to higherabsorption of objects in the south Galactic hemisphere or to atmospheric extinction in observations of clusters in high zenith angles.
dc.formatapplication/pdf
dc.languageeng
dc.publisherThe astronomical Journal
dc.relationcitation:Tovmassian, H. M., et al., (2008). On galactic absorption, The astronomical Journal. Vol.135(3):1067–1069
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/21
dc.titleOn galactic absorption
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


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