The morphology of CS Cha circumbinary disk suggesting the existence of a Saturn-mass planet

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dc.citation.articleNumberA151en_US
dc.citation.journalTitleAstronomy & Astrophysicsen_US
dc.citation.volumeNumber664en_US
dc.contributor.authorKurtovic, N.T.en_US
dc.contributor.authorPinilla, P.en_US
dc.contributor.authorPenzlin, Anna B.T.en_US
dc.contributor.authorBenisty, M.en_US
dc.contributor.authorPérez, L.en_US
dc.contributor.authorGinski, C.en_US
dc.contributor.authorIsella, A.en_US
dc.contributor.authorKley, W.en_US
dc.contributor.authorMenard, F.en_US
dc.contributor.authorPérez, S.en_US
dc.contributor.authorBayo, A.en_US
dc.date.accessioned2022-12-13T19:11:16Zen_US
dc.date.available2022-12-13T19:11:16Zen_US
dc.date.issued2022en_US
dc.description.abstractContext.Planets have been detected in circumbinary orbits in several different systems, despite the additional challenges faced during their formation in such an environment.Aims.We investigate the possibility of planetary formation in the spectroscopic binary CS Cha by analyzing its circumbinary disk.Methods. The system was studied with high angular resolution ALMA observations at 0.87 mm. Visibilities modeling and Keplerian fitting are used to constrain the physical properties of CS Cha, and the observations were compared to hydrodynamic simulations.Results.Our observations are able to resolve the disk cavity in the dust continuum emission and the 12CO J:3–2 transition. We find the dust continuum disk to be azimuthally axisymmetric (less than 9% of intensity variation along the ring) and of low eccentricity (of 0.039 at the peak brightness of the ring).Conclusions. Under certain conditions, low eccentricities can be achieved in simulated disks without the need of a planet, however, the combination of low eccentricity and axisymmetry is consistent with the presence of a Saturn-like planet orbiting near the edge of the cavity.en_US
dc.identifier.citationKurtovic, N.T., Pinilla, P., Penzlin, Anna B.T., et al.. "The morphology of CS Cha circumbinary disk suggesting the existence of a Saturn-mass planet." <i>Astronomy & Astrophysics,</i> 664, (2022) EDP Sciences: https://doi.org/10.1051/0004-6361/202243505.en_US
dc.identifier.digitalaa43505-22en_US
dc.identifier.doihttps://doi.org/10.1051/0004-6361/202243505en_US
dc.identifier.urihttps://hdl.handle.net/1911/114092en_US
dc.language.isoengen_US
dc.publisherEDP Sciencesen_US
dc.rightsOpen Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleThe morphology of CS Cha circumbinary disk suggesting the existence of a Saturn-mass planeten_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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