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http://hdl.handle.net/10261/147751
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Campo DC | Valor | Lengua/Idioma |
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dc.contributor.author | Costado, M. T. | es_ES |
dc.contributor.author | Alfaro, Emilio J. | es_ES |
dc.contributor.author | González García, Marta | es_ES |
dc.contributor.author | Sampedro, Laura | es_ES |
dc.date.accessioned | 2017-04-03T08:16:40Z | - |
dc.date.available | 2017-04-03T08:16:40Z | - |
dc.date.issued | 2016-11-17 | - |
dc.identifier.citation | Monthly Notices of the Royal Astronomical Society 465(4): 3879-3888 (2017) | es_ES |
dc.identifier.issn | 0035-8711 | - |
dc.identifier.uri | http://hdl.handle.net/10261/147751 | - |
dc.description.abstract | The main objective of this study is the characterization of the velocity field in the Cygnus OB1 association using the radial velocity data currently available in the literature. This association is part of a larger star-forming complex located in the direction of the Cygnus region, but whose main subsystems may be distributed at different distances from the sun. We have collected radial velocity data for more than 300 stars in the area of 5 × 5 deg2 centred on the Cygnus OB1 association. We present the results of a kinematic clustering analysis in the subspace of the phase space formed by angular coordinates and radial velocity using two independent methodologies. We have found evidence of structure in the phase space with the detection of two main groups, corresponding to different radial velocity and distance values, belonging to the association, and associated with two main shells defined by the Hα emission. A third grouping well separated from the other two in velocity appears to occupy the whole region associated with what has been called ‘common shell’.© 2016 The Authors. | es_ES |
dc.description.sponsorship | This work is financed by the Spanish Ministerio de Economia y Competitividad, through grant AYA2013-40611-P. This work makes use of EURO-VO software, tools or services. The EURO-VO has been funded by the European Commission through contracts RI031675 (DCA) and 011892 (VO-TECH) under the Sixth Framework Program and contracts 212104 (AIDA), 261541 (VOICE), 312559 (CoSADIE) under the Seventh Framework Program. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | Oxford University Press | es_ES |
dc.relation | info:eu-repo/grantAgreement/MINECO/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2013-40611-P | es_ES |
dc.relation | info:eu-repo/grantAgreement/EC/FP7/212104 | es_ES |
dc.relation | info:eu-repo/grantAgreement/EC/FP7/261541 | es_ES |
dc.relation | info:eu-repo/grantAgreement/EC/FP7/312559 | es_ES |
dc.relation.isversionof | Publisher's version | es_ES |
dc.rights | openAccess | es_ES |
dc.subject | Techniques: radial velocities | es_ES |
dc.subject | Stars: formation | es_ES |
dc.subject | Stars: kinematics and dynamics | es_ES |
dc.subject | Open clusters and associations: general | es_ES |
dc.title | Analysis of the kinematic structure of the Cygnus OB1 associatio | es_ES |
dc.type | artículo | es_ES |
dc.identifier.doi | 10.1093/mnras/stw2967 | - |
dc.description.peerreviewed | Peer reviewed | es_ES |
dc.relation.publisherversion | http://dx.doi.org/10.1093/mnras/stw2967 | es_ES |
dc.identifier.e-issn | 1365-2966 | - |
dc.contributor.funder | Ministerio de Economía y Competitividad (España) | es_ES |
dc.contributor.funder | European Commission | es_ES |
dc.relation.csic | Sí | es_ES |
oprm.item.hasRevision | no ko 0 false | * |
dc.identifier.funder | http://dx.doi.org/10.13039/501100003329 | es_ES |
dc.identifier.funder | http://dx.doi.org/10.13039/501100000780 | es_ES |
dc.type.coar | http://purl.org/coar/resource_type/c_6501 | es_ES |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | artículo | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
Aparece en las colecciones: | (IAA) Artículos |
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IAA_2017stw2967.pdf | 1,78 MB | Adobe PDF | Visualizar/Abrir |
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