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Investigating 2MASS J06593158-0405277 : a FUor burst in a triple system?

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dc.contributor.authorCaratti o Garatti, A.
dc.contributor.authorGarcia Lopez, R.
dc.contributor.authorRay, T. P.
dc.contributor.authorEislöffel, J.
dc.contributor.authorStecklum, B.
dc.contributor.authorScholz, A.
dc.contributor.authorKraus, S.
dc.contributor.authorWeigelt, G.
dc.contributor.authorKreplin, A.
dc.contributor.authorShenavrin, V.
dc.date.accessioned2016-04-13T15:30:03Z
dc.date.available2016-04-13T15:30:03Z
dc.date.issued2015-06-02
dc.identifier.citationCaratti o Garatti , A , Garcia Lopez , R , Ray , T P , Eislöffel , J , Stecklum , B , Scholz , A , Kraus , S , Weigelt , G , Kreplin , A & Shenavrin , V 2015 , ' Investigating 2MASS J06593158-0405277 : a FUor burst in a triple system? ' , Astrophysical Journal Letters , vol. 806 , no. 1 , L4 . https://doi.org/10.1088/2041-8205/806/1/L4en
dc.identifier.issn2041-8205
dc.identifier.otherPURE: 194132732
dc.identifier.otherPURE UUID: 9fd7c9aa-790e-43b9-b9fa-a75275dc3450
dc.identifier.otherBibCode: 2015arXiv150503691G
dc.identifier.otherBibCode: 2015ApJ...806L...4C
dc.identifier.otherArXiv: http://arxiv.org/abs/1505.03691v1
dc.identifier.otherScopus: 84930942557
dc.identifier.otherWOS: 000356633700004
dc.identifier.urihttp://hdl.handle.net/10023/8610
dc.descriptionA.C.G., R.G.L., and T.P.R. were supported by Science Foundation Ireland, grant 13/ERC/I2907. S.K. acknowledges support from an STFC Ernest Rutherford Fellowship (ST/J004030/1), Ernest Rutherford Grant (ST/K003445/1), and Marie Curie CIG grant (SH-06192).en
dc.description.abstractFUor outbursts in young stellar objects (YSOs) are the most dramatic events among episodic accretion phenomena. The origin of these bursts is not clear: disk instabilities and/or disk perturbations by an external body being the most viable hypotheses. Here, we report our VLT/SINFONI high angular resolution AO-assisted observations of 2MASSJ06593158-0405277, which is undergoing a recently discovered FUoroutburst. Our observations reveal the presence of an extended disc-like structure around the FUor, a very low-mass companion (2MASSJ06593158-0405277B) at ~100 au in projection, and, possibly, a third closer companion at ~11 au. These sources appear to be young, displaying accretion signatures. Assuming the components are physically linked,2MASS J06593158-0405277 would then be one of the very few triple systems observed in FUors.
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal Lettersen
dc.rights© 2015, American Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at iopscience.iop.org / https://dx.doi.org/10.1088/2041-8205/806/1/L4en
dc.subjectBinaries: closeen
dc.subjectCircumstellar matteren
dc.subjectStars: formationen
dc.subjectStars: individual: 2MASS J06593158-0405277en
dc.subjectStars: pre-main sequenceen
dc.subjectTechniques: high angular resolutionen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleInvestigating 2MASS J06593158-0405277 : a FUor burst in a triple system?en
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1088/2041-8205/806/1/L4
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2015arXiv150503691Gen


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