Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12666/234
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dc.rights.license© 2020. The American Astronomical Society. All rights reserved.-
dc.contributor.authorJiménez Serra, I.-
dc.contributor.authorBáez Rubio, A.-
dc.contributor.authorMartín Pintado, J.-
dc.contributor.authorZhang, Q.-
dc.contributor.authorRivilla, V. M.-
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737-
dc.date.accessioned2021-04-12T09:54:22Z-
dc.date.available2021-04-12T09:54:22Z-
dc.date.issued2020-07-13-
dc.identifier.citationThe Astrophysical Journal Letters 897(2): L33(2020)es
dc.identifier.issn0004-637X-
dc.identifier.otherhttps://iopscience.iop.org/article/10.3847/2041-8213/aba050-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/234-
dc.description.abstractTheories of massive star formation predict that massive protostars accrete gas through circumstellar disks. Although several cases have been found already thanks to high angular-resolution interferometry, the internal physical structure of these disks remains unknown, in particular whether they present warps or internal holes, as observed in low-mass protoplanetary disks. Here, we report very high angular-resolution observations of the H21 alpha radio recombination line carried out in Band 9 with the Atacama Large Millimeter/submillimeter Array (beam of 80 mas x 60 mas, or 70 au x 50 au) toward the IRS2 massive young stellar object in the Monoceros R2 star-forming cluster. The H21 alpha line shows maser amplification, which allows us to study the kinematics and physical structure of the ionized gas around the massive protostar down to spatial scales of similar to 1-2 au. Our ALMA images and 3D radiative transfer modeling reveal that the ionized gas around IRS2 is distributed in a Keplerian circumstellar disk and an expanding wind. The H21 alpha emission centroids at velocities between -10 and 20 km s(-1)deviate from the disk plane, suggesting a warping for the disk. This could be explained by the presence of a secondary object (a stellar companion or a massive planet) within the system. The ionized wind seems to be launched from the disk surface at distances similar to 11 au from the central star, consistent with magnetically-regulated disk wind models. This suggests a similar wind-launching mechanism to that recently found for evolved massive stars such as MWC349A and MWC922.es
dc.description.sponsorshipWe thank the anonymous referee for the constructive comments. This Letter makes use of the ALMA data ADS/JAO.ALMA 2012.1.00522.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. I.J.-S., A.B.-R., and J.M.-P. acknowledge support from the Spanish FEDER (project number ESP2017-86582-C4-1-R) and the State Research Agency (AEI; project number PID2019-105552RB-C41). V.M.R. has received funding from the EU Horizon 2020 program under the Marie Sklodowska-Curie grant agreement No. 664931. We thank A. Richards for the help provided during the calibration/imaging of the data; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737).es
dc.language.isoenges
dc.publisherThe Institute of Physics (IOP)es
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2017-86582-C4-1-R/ES/CONTRIBUCION ESPAÑOLA A LAS MISIONES ESPACIALES CRIOGENICAS SPICA Y ATHENA, POST-OPERACIONES DE HERSCHEL Y EXPLOTACION CIENTIFICA MULTIFRECUENCIA/-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105552RB-C41/ES/CONTRIBUCION DEL CAB A SPICA, DESARROLLO DE INSTRUMENTACION CRIOGENICA Y EXPLOTACION CIENTIFICA MULTILONGITUD DE ONDA/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internationales
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/-
dc.subjectStar formationes
dc.titleThe Ionized Warped Disk and Disk Wind of the Massive Protostar Monoceros R2-IRS2 Seen with ALMAes
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidJiménez Serra, I. [0000-0003-4493-8714]-
dc.contributor.orcidZhang, Q. [0000-0003-2384-6589]-
dc.contributor.orcidRivilla, V. M. [0000-0002-2887-5859]-
dc.identifier.doi10.3847/2041-8213/aba050-
dc.identifier.e-issn1538-4357-
dc.contributor.funderAgencia Estatal de Investigación (AEI)-
dc.contributor.funderEuropean Research Council (ERC)-
dc.description.peerreviewedPeer reviewes
dc.identifier.funderhttp://dx.doi.org/10.13039/501100011033-
dc.identifier.funderhttp://dx.doi.org/10.13039/501100000781-
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/664931-
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