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dc.contributor.authorLi, TKen_US
dc.contributor.authorTar, JJMen_US
dc.contributor.authorHsu, LHen_US
dc.date.accessioned2014-12-08T15:38:32Z-
dc.date.available2014-12-08T15:38:32Z-
dc.date.issued2004-09-03en_US
dc.identifier.issn0020-0255en_US
dc.identifier.urihttp://dx.doi.org/10.1016/j.ins.2003.09.023en_US
dc.identifier.urihttp://hdl.handle.net/11536/26383-
dc.description.abstractThe star graph posses many nice topological properties. Edge fault tolerance is an important issue for a network since the edges in the network may fail sometimes. In this paper, we show that the n-dimensional star graph is (n - 3)-edge fault tolerant hamiltonian laceable, (n - 3)-edge fault tolerant strongly hamiltonian laceable, and (n - 4)-edge fault tolerant hyper hamiltonian laceable. All these results are optimal in a sense described in this paper. (C) 2003 Elsevier Inc. All rights reserved.en_US
dc.language.isoen_USen_US
dc.subjectstar graphen_US
dc.subjecthamiltonian laceableen_US
dc.subjectstrongly hamiltonian laceableen_US
dc.subjecthyper hamiltonian laceableen_US
dc.subjectfault toleranten_US
dc.titleHyper hamiltonian laceability on edge fault star graphen_US
dc.typeArticleen_US
dc.identifier.doi10.1016/j.ins.2003.09.023en_US
dc.identifier.journalINFORMATION SCIENCESen_US
dc.citation.volume165en_US
dc.citation.issue1-2en_US
dc.citation.spage59en_US
dc.citation.epage71en_US
dc.contributor.department資訊工程學系zh_TW
dc.contributor.departmentDepartment of Computer Scienceen_US
dc.identifier.wosnumberWOS:000223749900004-
dc.citation.woscount50-
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