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dc.contributor.authorKohn, Saul A.
dc.contributor.authorShkolnik, Evgenya L.
dc.contributor.authorWeinberger, Alycia J.
dc.contributor.authorCarlberg, Joleen K.
dc.contributor.authorLlama, Joe
dc.date.accessioned2016-03-30T11:30:13Z
dc.date.available2016-03-30T11:30:13Z
dc.date.issued2016-03-10
dc.identifier.citationKohn , S A , Shkolnik , E L , Weinberger , A J , Carlberg , J K & Llama , J 2016 , ' Searching for spectroscopic binaries within transition disk objects ' , Astrophysical Journal , vol. 820 , no. 1 , pp. 1-15 . https://doi.org/10.3847/0004-637X/820/1/2en
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 241226297
dc.identifier.otherPURE UUID: 46ef86c3-5d15-44db-b39b-0701dbb9d6ee
dc.identifier.otherArXiv: http://arxiv.org/abs/1602.07582v1
dc.identifier.otherScopus: 84962282061
dc.identifier.otherWOS: 000372787000002
dc.identifier.urihttp://hdl.handle.net/10023/8516
dc.descriptionS.A. Kohn acknowledges the support of NSF REU grant AST-1004107 through Northern Arizona University and Lowell Observatory. J. Llama acknowledges support from NASA Origins of the Solar System grant No. NNX13AH79G and from STFC grant ST/M001296/1. This research made use of the SIMBAD database, operated at CDS, Strasbourg, France.en
dc.description.abstractTransition disks (TDs) are intermediate stage circumstellar disks characterized by an inner gap within the disk structure. To test whether these gaps may have been formed by closely orbiting, previously undetected stellar companions, we collected high-resolution optical spectra of 31 TD objects to search for spectroscopic binaries (SBs). Twenty-four of these objects are in Ophiuchus and seven are within the Coronet, Corona Australis, and Chameleon I star-forming regions. We measured radial velocities for multiple epochs, obtaining a median precision of 400 ms−1. We identified double-lined SB SSTc2d J163154.7–250324 in Ophiuchus, which we determined to be composed of a K7(±0.5) and a K9(±0.5) star, with orbital limits of a < 0.6 au and P < 150 days. This results in an SB fraction of in Ophiuchus, which is consistent with other spectroscopic surveys of non-TD objects in the region. This similarity suggests that TDs are not preferentially sculpted by the presence of close binaries and that planet formation around close binaries may take place over similar timescales to that around single stars.
dc.format.extent15
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2016. The American Astronomical Society. All rights reserved. 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/10.3847/0004-637X/820/1/2en
dc.subjectBinariesen
dc.subjectSpectroscopicen
dc.subjectCircumstellar matteren
dc.subjectStars: pre-main sequenceen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleSearching for spectroscopic binaries within transition disk objectsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.3847/0004-637X/820/1/2
dc.description.statusPeer revieweden
dc.identifier.urlhttp://arxiv.org/abs/1602.07582en


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