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dc.contributor.authorTifft, W. G.
dc.contributor.authorConnolly, L. P.
dc.contributor.authorWebb, D. F.
dc.date.accessioned2018-04-06T16:30:24Z
dc.date.available2018-04-06T16:30:24Z
dc.date.issued1971-12
dc.identifier.citationMNRAS 158: 47-62 (1972)en_US
dc.identifier.urihttp://hdl.handle.net/10150/627227
dc.description.abstractThree color UBV photometry of the cluster NGC 2818 shows it to lie at a distance of 3.2 kpc. The cluster has a color excess E_(B-V)= 0.22 and an ultraviolet excess of 0.09. The evolutionary turnoff from the main sequence occurs in mid A. The faint main sequence in the cluster shows a distinct bend or discontinuity. Preliminary velocity measurements indicate that the high excitation planetary nebula NGC 2818 is probably associated with the cluster.en_US
dc.language.isoen_USen_US
dc.publisherSteward Observatory, The University of Arizona (Tucson, Arizona)en_US
dc.relation.ispartofseriesPreprints of the Steward Observatory #0041en_US
dc.relation.urlhttp://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1972MNRAS.158...47T&db_key=AST&data_type=HTML&format=&high=3ed65e9cd019379en_US
dc.rightsCopyright © All Rights Reserved.en_US
dc.sourceSteward Observatory Parker Library SO QB 4 .S752 ARCHen_US
dc.subjectOpen star clustersen_US
dc.subjectPlanetary nebulaeen_US
dc.subjectJohnson photometryen_US
dc.titleNGC 2818, An Open Cluster containing a Planetary Nebulaeen_US
dc.typetexten_US
dc.contributor.departmentUniv Arizona, Steward Observen_US
dc.description.collectioninformationThis title from the Steward Observatory Preprints collection is made available by the Steward Observatory Parker Library and the University Libraries, The University of Arizona. If you have questions about titles in this collection, please contact Parker Library librarian Betty Fridena, bfridena@as.arizona.edu.en_US
refterms.dateFOA2018-04-06T16:30:24Z


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