The candidate 31.4 day periodicity from Cyg X-3 is an artifact of ASM data sampling

dc.contributor.authorTomsick, John A.
dc.contributor.authorVilhu, Osmi
dc.contributor.authorWilms, Joern
dc.contributor.authorBodaghee, Arash
dc.contributor.authorPottschmidt, Katja
dc.contributor.authorRodriguez, Jerome
dc.contributor.authorLevine, Al
dc.contributor.authorHakala, Pasi
dc.contributor.authorHannikainen, Diana
dc.date.accessioned2023-09-22T16:09:07Z
dc.date.available2023-09-22T16:09:07Z
dc.date.issued2011-06-17
dc.description.urihttps://astronomerstelegram.org/?read=3437en
dc.genrearticlesen
dc.identifierdoi:10.13016/m2uwji-fbts
dc.identifier.citationTomsick, J. A. et al. “The candidate 31.4 day periodicity from Cyg X-3 is an artifact of ASM data sampling”. ATel.3437 (17 Jun 2011). https://astronomerstelegram.org/?read=3437en
dc.identifier.urihttp://hdl.handle.net/11603/29835
dc.language.isoenen
dc.publisherThe Astronomer's Telegramen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Center for Space Sciences and Technology
dc.relation.ispartofUMBC Physics Department
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.en
dc.subjectX-rayen
dc.subjectBinaryen
dc.subjectBlack Holeen
dc.subjectNeutron Staren
dc.subjectVariablesen
dc.titleThe candidate 31.4 day periodicity from Cyg X-3 is an artifact of ASM data samplingen
dc.typeTexten
dcterms.creatorhttps://orcid.org/0000-0002-4656-6881en

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