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Nielsen, Martin Bo
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Nielsen, Martin Bo
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Nielsen, Martin Bo
Alternative Name
Nielsen, Martin B.
Nielsen, M. B.
Nielsen, Martin
Nielsen, M.
Now showing 1 - 5 of 5
2018Journal Article [["dc.bibliographiccitation.firstpage","119"],["dc.bibliographiccitation.issue","2"],["dc.bibliographiccitation.journal","The Astrophysical Journal"],["dc.bibliographiccitation.volume","857"],["dc.contributor.author","Benomar, O."],["dc.contributor.author","Goupil, Mjo."],["dc.contributor.author","Belkacem, K."],["dc.contributor.author","Appourchaux, T."],["dc.contributor.author","Nielsen, M. B."],["dc.contributor.author","Bazot, M."],["dc.contributor.author","Gizon, Laurent"],["dc.contributor.author","Hanasoge, S."],["dc.contributor.author","Sreenivasan, K. R."],["dc.contributor.author","Marchand, B."],["dc.date.accessioned","2020-12-10T18:47:34Z"],["dc.date.available","2020-12-10T18:47:34Z"],["dc.date.issued","2018"],["dc.identifier.doi","10.3847/1538-4357/aab9b7"],["dc.identifier.eissn","1538-4357"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/78809"],["dc.notes.intern","DOI Import GROB-354"],["dc.title","Asymmetry of Line Profiles of Stellar Oscillations Measured by Kepler for Ensembles of Solar-like Oscillators: Impact on Mode Frequencies and Dependence on Effective Temperature"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2018Journal Article [["dc.bibliographiccitation.firstpage","L9"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.volume","619"],["dc.contributor.author","Bazot, M."],["dc.contributor.author","Nielsen, M. B."],["dc.contributor.author","Mary, D."],["dc.contributor.author","Christensen-Dalsgaard, J."],["dc.contributor.author","Benomar, O."],["dc.contributor.author","Petit, P."],["dc.contributor.author","Gizon, Laurent"],["dc.contributor.author","Sreenivasan, K. R."],["dc.contributor.author","White, T. R."],["dc.date.accessioned","2020-12-10T18:11:44Z"],["dc.date.available","2020-12-10T18:11:44Z"],["dc.date.issued","2018"],["dc.identifier.doi","10.1051/0004-6361/201834251"],["dc.identifier.eissn","1432-0746"],["dc.identifier.issn","0004-6361"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/74126"],["dc.notes.intern","DOI Import GROB-354"],["dc.title","Butterfly diagram of a Sun-like star observed using asteroseismology"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2019Journal Article [["dc.bibliographiccitation.firstpage","A125"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.volume","623"],["dc.contributor.author","Bazot, M."],["dc.contributor.author","Benomar, O."],["dc.contributor.author","Christensen-Dalsgaard, J."],["dc.contributor.author","Gizon, Laurent"],["dc.contributor.author","Hanasoge, S."],["dc.contributor.author","Nielsen, M."],["dc.contributor.author","Petit, P."],["dc.contributor.author","Sreenivasan, K. R."],["dc.date.accessioned","2020-12-10T18:11:45Z"],["dc.date.available","2020-12-10T18:11:45Z"],["dc.date.issued","2019"],["dc.identifier.doi","10.1051/0004-6361/201834594"],["dc.identifier.eissn","1432-0746"],["dc.identifier.issn","0004-6361"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/74132"],["dc.notes.intern","DOI Import GROB-354"],["dc.title","Latitudinal differential rotation in the solar analogues 16 Cygni A and B"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI2017Journal Article [["dc.bibliographiccitation.artnumber","A82"],["dc.bibliographiccitation.journal","Astronomy and Astrophysics"],["dc.bibliographiccitation.volume","601"],["dc.contributor.author","White, Timothy R."],["dc.contributor.author","Benomar, O."],["dc.contributor.author","Aguirre, Victor Silva"],["dc.contributor.author","Ball, Warrick H."],["dc.contributor.author","Bedding, Timothy R."],["dc.contributor.author","Chaplin, W. J."],["dc.contributor.author","Christensen-Dalsgaard, Joergen"],["dc.contributor.author","Garcia, R. A."],["dc.contributor.author","Gizon, Laurent"],["dc.contributor.author","Stello, Dennis"],["dc.contributor.author","Aigrain, S."],["dc.contributor.author","Antia, H. M."],["dc.contributor.author","Appourchaux, T."],["dc.contributor.author","Bazot, M."],["dc.contributor.author","Campante, Tiago L."],["dc.contributor.author","Creevey, O. L."],["dc.contributor.author","Davies, G. R."],["dc.contributor.author","Elsworth, Yvonne P."],["dc.contributor.author","Gaulme, P."],["dc.contributor.author","Handberg, Rasmus"],["dc.contributor.author","Hekker, Saskia"],["dc.contributor.author","Houdek, Gunter"],["dc.contributor.author","Howe, R."],["dc.contributor.author","Huber, D."],["dc.contributor.author","Karoff, Christoffer"],["dc.contributor.author","Marques, J. P."],["dc.contributor.author","Mathur, S."],["dc.contributor.author","McQuillan, A."],["dc.contributor.author","Metcalfe, T. S."],["dc.contributor.author","Mosser, B."],["dc.contributor.author","Nielsen, M. B."],["dc.contributor.author","Regulo, C."],["dc.contributor.author","Salabert, D."],["dc.contributor.author","Stahn, Thorsten"],["dc.date.accessioned","2018-11-07T10:24:05Z"],["dc.date.available","2018-11-07T10:24:05Z"],["dc.date.issued","2017"],["dc.description.abstract","Binary star systems are important for understanding stellar structure and evolution, and are especially useful when oscillations can be detected and analysed with asteroseismology. However, only four systems are known in which solar-like oscillations are detected in both components. Here, we analyse the fifth such system, HD 176465, which was observed by Kepler. We carefully analysed the system's power spectrum to measure individual mode frequencies, adapting our methods where necessary to accommodate the fact that both stars oscillate in a similar frequency range. We also modelled the two stars independently by fitting stellar models to the frequencies and complementary parameters. We are able to cleanly separate the oscillation modes in both systems. The stellar models produce compatible ages and initial compositions for the stars, as is expected from their common and contemporaneous origin. Combining the individual ages, the system is about 3.0 +/- 0.5 Gyr old. The two components of HD 176465 are young physically-similar oscillating solar analogues, the first such system to be found, and provide important constraints for stellar evolution and asteroseismology."],["dc.identifier.doi","10.1051/0004-6361/201628706"],["dc.identifier.isi","000402313500082"],["dc.identifier.purl","https://resolver.sub.uni-goettingen.de/purl?gs-1/15004"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/42591"],["dc.notes.intern","Merged from goescholar"],["dc.notes.status","zu prüfen"],["dc.notes.submitter","PUB_WoS_Import"],["dc.publisher","Edp Sciences S A"],["dc.relation","info:eu-repo/grantAgreement/EC/FP7/338251/EU//STELLARAGES"],["dc.relation.issn","1432-0746"],["dc.relation.orgunit","Fakultät für Physik"],["dc.title","Kepler observations of the asteroseismic binary HD 176465"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dc.type.peerReviewed","yes"],["dc.type.status","published"],["dc.type.version","published_version"],["dspace.entity.type","Publication"]]Details DOI WOS2018Journal Article [["dc.bibliographiccitation.firstpage","1231"],["dc.bibliographiccitation.issue","6408"],["dc.bibliographiccitation.journal","Science"],["dc.bibliographiccitation.lastpage","1234"],["dc.bibliographiccitation.volume","361"],["dc.contributor.author","Benomar, O."],["dc.contributor.author","Bazot, M."],["dc.contributor.author","Nielsen, M. B."],["dc.contributor.author","Gizon, Laurent"],["dc.contributor.author","Sekii, T."],["dc.contributor.author","Takata, M."],["dc.contributor.author","Hotta, H."],["dc.contributor.author","Hanasoge, S."],["dc.contributor.author","Sreenivasan, K. R."],["dc.contributor.author","Christensen-Dalsgaard, J."],["dc.date.accessioned","2020-12-10T18:36:43Z"],["dc.date.available","2020-12-10T18:36:43Z"],["dc.date.issued","2018"],["dc.identifier.doi","10.1126/science.aao6571"],["dc.identifier.eissn","1095-9203"],["dc.identifier.issn","0036-8075"],["dc.identifier.uri","https://resolver.sub.uni-goettingen.de/purl?gro-2/76717"],["dc.language.iso","en"],["dc.notes.intern","DOI Import GROB-354"],["dc.title","Asteroseismic detection of latitudinal differential rotation in 13 Sun-like stars"],["dc.type","journal_article"],["dc.type.internalPublication","yes"],["dspace.entity.type","Publication"]]Details DOI