dc.contributor.author | Reed, Michael D | |
dc.contributor.author | Armbrecht, EL | |
dc.contributor.author | Telting, John H | |
dc.contributor.author | Baran, Andrzej S | |
dc.contributor.author | Østensen, Roy | |
dc.contributor.author | Blay, Pere | |
dc.contributor.author | Kvammen, Andreas | |
dc.contributor.author | Kuutma, Teet | |
dc.contributor.author | Pursimo, Tapio | |
dc.contributor.author | Ketzer, Laura | |
dc.contributor.author | Jeffery, C. Simon | |
dc.date.accessioned | 2019-02-20T13:52:46Z | |
dc.date.available | 2019-02-20T13:52:46Z | |
dc.date.issued | 2017-12-05 | |
dc.description.abstract | We report the discovery of three pulsating subdwarf B stars in binary systems observed with the <i>Kepler</i> space telescope during Campaign 5 of K2. EPIC 211696659 (SDSS J083603.98+155216.4) is a g-mode pulsator with a white dwarf companion and a binary period of 3.16 d. EPICs 211823779 (SDSS J082003.35+173914.2) and 211938328 (LB 378) are both p-mode pulsators with main-sequence F companions. The orbit of EPIC 211938328 is long (635 ± 146 d) while we cannot constrain that of EPIC 211823779. The p modes are near the Nyquist frequency and so we investigate ways to discriminate super- from sub-Nyquist frequencies. We search for rotationally induced frequency multiplets and all three stars appear to be slow rotators with EPIC 211696659 subsynchronous to its orbit. | en_US |
dc.description.sponsorship | The National Science Foundation
The Polish National Science Center
The NASA Science Mission directorate
The NASA Office of Space Science | en_US |
dc.description | This article has been accepted for publication in <i>Monthly notices of the Royal Astronomical Society</i> ©: 2018 Royal Astronomical Society. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. The version of record Reed, M.D., Armbrecht, E.L., Telting, J.H., Baran, A.S., Østensen, R., Blay, P., ... Jeffery, C.S. (2018). K2 Campaign 5 observations of pulsating subdwarf B stars: Binaries and super-Nyquist frequencies. <i>Monthly notices of the Royal Astronomical Society, 474</i>(4), 5186-5198 is available online at: <a href=https://doi.org/10.1093/mnras/stx3133> https://doi.org/10.1093/mnras/stx3133</a>. | en_US |
dc.identifier.citation | Reed, M.D., Armbrecht, E.L., Telting, J.H., Baran, A.S., Østensen, R., Blay, P., ... Jeffery, C.S. (2018). K2 Campaign 5 observations of pulsating subdwarf B stars: Binaries and super-Nyquist frequencies. <i>Monthly notices of the Royal Astronomical Society, 474</i>(4), 5186-5198. https://doi.org/10.1093/mnras/stx3133 | en_US |
dc.identifier.cristinID | FRIDAID 1627392 | |
dc.identifier.doi | 10.1093/mnras/stx3133 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.issn | 1365-2966 | |
dc.identifier.uri | https://hdl.handle.net/10037/14731 | |
dc.language.iso | eng | en_US |
dc.publisher | Oxford University Press (OUP) | en_US |
dc.relation.journal | Monthly notices of the Royal Astronomical Society | |
dc.rights.accessRights | openAccess | en_US |
dc.subject | VDP::Mathematics and natural science: 400::Physics: 430::Space and plasma physics: 437 | en_US |
dc.subject | VDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Rom- og plasmafysikk: 437 | en_US |
dc.title | K2 Campaign 5 observations of pulsating subdwarf B stars: Binaries and super-Nyquist frequencies | en_US |
dc.type | Journal article | en_US |
dc.type | Tidsskriftartikkel | en_US |
dc.type | Peer reviewed | en_US |