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Fault Hamiltonicity and fault Hamiltonian connectivity of the (n, k)-star graphs

dc.citation.epage201en_US
dc.citation.issue4en_US
dc.citation.spage189en_US
dc.citation.volume42en_US
dc.citation.woscount29
dc.contributor.authorHsu, HCen_US
dc.contributor.authorHsieh, YLen_US
dc.contributor.authorTan, JJMen_US
dc.contributor.authorHsu, LHen_US
dc.contributor.department資訊工程學系zh_TW
dc.contributor.departmentDepartment of Computer Scienceen_US
dc.date.accessioned2014-12-08T15:40:02Z
dc.date.available2014-12-08T15:40:02Z
dc.date.issued2003-12-01en_US
dc.description.abstractIn this paper, we consider the fault Hamiltonicity, and the fault Hamiltonian connectivity of the (n, k)-star graph S-n,S-k. Assume that F subset of V(S-n,S-k) boolean OR E(S-n,S-k). For n - k greater than or equal to 2, we prove that S-n,S-k - F is Hamiltonian if F less than or equal to n - 3 and S-n,S-k - F is Hamiltonian connected if F less than or equal to n - 4. For n - k = 1, S-n,S-n-1 is isomorphic to the n-star graph S-n which is known to be Hamiltonian if and only if n > 2 and Hamiltonian connected if and only if n = 2. Moreover, all the bounds are tight. (C) 2003 Wiley Periodicals, Inc.en_US
dc.identifier.doi10.1002/net.10096en_US
dc.identifier.issn0028-3045en_US
dc.identifier.journalNETWORKSen_US
dc.identifier.urihttp://dx.doi.org/10.1002/net.10096en_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/27348
dc.identifier.wosnumberWOS:000186619700002
dc.language.isoen_USen_US
dc.subjectHamiltonian cycleen_US
dc.subjectHamiltonian connecteden_US
dc.subject(n, k)-star graphen_US
dc.titleFault Hamiltonicity and fault Hamiltonian connectivity of the (n, k)-star graphsen_US
dc.typeArticleen_US

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