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Article: Correlation effects in microwave observations of selected RS CVn-like stars

TitleCorrelation effects in microwave observations of selected RS CVn-like stars
Authors
Budding, ELim, JSlee, OBWhite, SM
KeywordsBinaries: Close
Cf Tucanae
Radio Continuum: Stars
Stars: Activity
Stars: Coronae
Stars: Individual
Stars: Individual: Ab Doradus
Stars: Individual: Au Microscopii
Stars: Individual: Hr 1099
Stars: Individual: V824 Arae
Techniques: Miscellaneous
Issue Date2002
PublisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/newast
Citation
New Astronomy, 2002, v. 7 n. 1, p. 35-43 How to Cite?
AbstractSets of dual frequency microwave data on selected chromospherically active stars, from the Australia Telescope Compact Array, have been investigated for their auto and cross-correlation effects. Comparison of cross-correlation peak values with theoretical expectation indicates a high degree of real physical connection between the emission at the pairs of frequencies (4.8 and 8.64 GHz) compared. This fact should help constrain models for the emission mechanism. The timescale of observed time-shifts between the emissions at the two frequencies is consistent, in general, with the underlying energization being propagated by magnetohydrodynamic waves in a compact turbulent medium. © 2002 Elsevier Science B.V. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/174991
ISSN
1384-1076
2021 Impact Factor: 2.096
2020 SCImago Journal Rankings: 0.435
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorBudding, Een_US
dc.contributor.authorLim, Jen_US
dc.contributor.authorSlee, OBen_US
dc.contributor.authorWhite, SMen_US
dc.date.accessioned2012-11-26T08:48:40Z-
dc.date.available2012-11-26T08:48:40Z-
dc.date.issued2002en_US
dc.identifier.citationNew Astronomy, 2002, v. 7 n. 1, p. 35-43en_US
dc.identifier.issn1384-1076en_US
dc.identifier.urihttp://hdl.handle.net/10722/174991-
dc.description.abstractSets of dual frequency microwave data on selected chromospherically active stars, from the Australia Telescope Compact Array, have been investigated for their auto and cross-correlation effects. Comparison of cross-correlation peak values with theoretical expectation indicates a high degree of real physical connection between the emission at the pairs of frequencies (4.8 and 8.64 GHz) compared. This fact should help constrain models for the emission mechanism. The timescale of observed time-shifts between the emissions at the two frequencies is consistent, in general, with the underlying energization being propagated by magnetohydrodynamic waves in a compact turbulent medium. © 2002 Elsevier Science B.V. All rights reserved.en_US
dc.languageengen_US
dc.publisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/newasten_US
dc.relation.ispartofNew Astronomyen_US
dc.subjectBinaries: Closeen_US
dc.subjectCf Tucanaeen_US
dc.subjectRadio Continuum: Starsen_US
dc.subjectStars: Activityen_US
dc.subjectStars: Coronaeen_US
dc.subjectStars: Individualen_US
dc.subjectStars: Individual: Ab Doradusen_US
dc.subjectStars: Individual: Au Microscopiien_US
dc.subjectStars: Individual: Hr 1099en_US
dc.subjectStars: Individual: V824 Araeen_US
dc.subjectTechniques: Miscellaneousen_US
dc.titleCorrelation effects in microwave observations of selected RS CVn-like starsen_US
dc.typeArticleen_US
dc.identifier.emailLim, J: jjlim@hku.hken_US
dc.identifier.authorityLim, J=rp00745en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.scopuseid_2-s2.0-31244435830en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-31244435830&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume7en_US
dc.identifier.issue1en_US
dc.identifier.spage35en_US
dc.identifier.epage43en_US
dc.publisher.placeNetherlandsen_US
dc.identifier.scopusauthoridBudding, E=7003577778en_US
dc.identifier.scopusauthoridLim, J=7403453870en_US
dc.identifier.scopusauthoridSlee, OB=6602225973en_US
dc.identifier.scopusauthoridWhite, SM=7404079906en_US
dc.identifier.issnl1384-1076-

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