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dc.date.accessioned 2019-10-31T14:57:42Z
dc.date.available 2019-10-31T14:57:42Z
dc.date.issued 2008
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/84542
dc.description.abstract We have analysed spectra obtained with the Gemini Multi Object Spectrograph (GMOS) for more than 50 stars in the ionising cluster of 30Doradus during a seven epochs observing campaign at Gemini South. We derive a binary candidate rate of about 50%, which is however consistent with an intrinsic 100% binary rate among massive stars. After decontaminating the sample from the stars that show binary orbital motions, we were able to calculate the "true" cluster velocity dispersion and found it to be about 8 km s-1. This value implies a virial mass of about 4.5 × 10M⊙ which is consistent with previous photometric mass determinations therefore suggesting that NGC 2070 is a firm candidate for a future globular cluster. en
dc.format.extent 317-322 es
dc.language en es
dc.subject Binaries: spectroscopic es
dc.subject Galaxies: individual (LMC) es
dc.subject Magellanic Clouds es
dc.subject Stars: early-type es
dc.subject Stars: kinematics es
dc.title Gemini/GMOS detection of stellar velocity variations in the ionising cluster of 30 Dor en
dc.type Articulo es
sedici.identifier.other doi:10.1017/S1743921308028640 es
sedici.identifier.other eid:2-s2.0-84884895778 es
sedici.identifier.issn 1743-9213 es
sedici.creator.person Bosch, Guillermo Luis es
sedici.creator.person Terlevich, Elena es
sedici.creator.person Terlevich, Roberto es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Facultad de Ciencias Astronómicas y Geofísicas es
sedici.subtype Articulo es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.relation.event IAU Symposium 256 (Keele, Staffordshire, UK, July 28-August 1, 2008) es
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Proceedings of the International Astronomical Union es
sedici.relation.journalVolumeAndIssue vol. 4, no. S256 es
sedici.rights.sherpa * RoMEO: verde* Pre-print del autor: can* Post-print del autor: can* Versión de editor/PDF:cannot* Condiciones:>>Author's Pre-print on author's personal website, departmental website, social media websites, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv>>Author's post-print on author's personal website on acceptance of publication>>Author's post-print on departmental website, institutional repository, non-commercial subject-based repositories, such as PubMed Central, Europe PMC or arXiv, after a 6 months embargo>>La versión de editor/PDF no puede utilizarse>>Published abstract may be deposited>>El pre-print debe registrar la aceptación para su publicación>>Deben reconocerse el copyright y la fuente editorial>>Must link to publisher version or journal website>>Authors may choose to use a Creative Commons Attribution Non-Commercial No Derivatives License>>Publisher last reviewed on 09/10/2014* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/1743-9213/es/


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)