Show simple item record

Files in this item

Item metadata

dc.contributor.authorXiang, Yue
dc.contributor.authorGu, Shenghong
dc.contributor.authorCameron, Andrew Collier
dc.contributor.authorBarnes, John Robert
dc.contributor.authorZhang, Liyun
dc.date.accessioned2016-02-04T17:10:09Z
dc.date.available2016-02-04T17:10:09Z
dc.date.issued2016-02-11
dc.identifier.citationXiang , Y , Gu , S , Cameron , A C , Barnes , J R & Zhang , L 2016 , ' The first Doppler images of the eclipsing binary SZ Piscium ' Monthly Notices of the Royal Astronomical Society , vol 456 , no. 1 , pp. 314-322 . DOI: 10.1093/mnras/stv2642en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 240446760
dc.identifier.otherPURE UUID: 22c4266c-5d47-45d1-ae7d-76f96d9aa612
dc.identifier.otherBibCode: 2016MNRAS.456..314X
dc.identifier.otherScopus: 84959464361
dc.identifier.urihttp://hdl.handle.net/10023/8135
dc.identifier.urihttp://mnras.oxfordjournals.org/content/456/1/314/suppl/DC1en
dc.identifier.urihttp://adsabs.harvard.edu/abs/2016MNRAS.456..314Xen
dc.description.abstractWe present the first Doppler images of the active eclipsing binary system SZ Psc, based on the high-resolution spectral data sets obtained in 2004 November and 2006 September-December. The least-squares deconvolution technique was applied to derive high signal-to-noise profiles from the observed spectra of SZ Psc. Absorption features contributed by a third component of the system were detected in the LSD profiles at all observed phases. We estimated the mass and period of the third component to be about 0.9 M⊙ and 1283 ± 10 d, respectively. After removing the contribution of the third body from the least-squares deconvolved profiles, we derived the surface maps of SZ Psc. The resulting Doppler images indicate significant star-spot activities on the surface of the K subgiant component. The distributions of star-spots are more complex than that revealed by previous photometric studies. The cooler K component exhibited pronounced high-latitude spots as well as numerous low- and intermediate-latitude spot groups during the entire observing seasons, but did not show any large, stable polar cap, different from many other active RS CVn-type binaries.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2015 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at https://dx.doi.org/10.1093/mnras/stv2642en
dc.subjectStars: activityen
dc.subjectBinaries: eclipsingen
dc.subjectStars: imagingen
dc.subjectStars: individual: SZ Pscen
dc.subjectStarspotsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe first Doppler images of the eclipsing binary SZ Pisciumen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stv2642
dc.description.statusPeer revieweden


The following license files are associated with this item:

This item appears in the following Collection(s)

Show simple item record