Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Hsu, HC | en_US |
dc.contributor.author | Hsieh, YL | en_US |
dc.contributor.author | Tan, JJM | en_US |
dc.contributor.author | Hsu, LH | en_US |
dc.date.accessioned | 2014-12-08T15:40:02Z | - |
dc.date.available | 2014-12-08T15:40:02Z | - |
dc.date.issued | 2003-12-01 | en_US |
dc.identifier.issn | 0028-3045 | en_US |
dc.identifier.uri | http://dx.doi.org/10.1002/net.10096 | en_US |
dc.identifier.uri | http://hdl.handle.net/11536/27348 | - |
dc.description.abstract | In 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.language.iso | en_US | en_US |
dc.subject | Hamiltonian cycle | en_US |
dc.subject | Hamiltonian connected | en_US |
dc.subject | (n, k)-star graph | en_US |
dc.title | Fault Hamiltonicity and fault Hamiltonian connectivity of the (n, k)-star graphs | en_US |
dc.type | Article | en_US |
dc.identifier.doi | 10.1002/net.10096 | en_US |
dc.identifier.journal | NETWORKS | en_US |
dc.citation.volume | 42 | en_US |
dc.citation.issue | 4 | en_US |
dc.citation.spage | 189 | en_US |
dc.citation.epage | 201 | en_US |
dc.contributor.department | 資訊工程學系 | zh_TW |
dc.contributor.department | Department of Computer Science | en_US |
dc.identifier.wosnumber | WOS:000186619700002 | - |
dc.citation.woscount | 29 | - |
Appears in Collections: | Articles |
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