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dc.date.accessioned | 2019-10-31T13:53:50Z | |
dc.date.available | 2019-10-31T13:53:50Z | |
dc.date.issued | 2003 | |
dc.identifier.uri | http://sedici.unlp.edu.ar/handle/10915/84494 | |
dc.description.abstract | We present the first linear multicolor polarization observations for a sample of 35 stars in the direction of the Galactic cluster NGC 6231. We have found a complex pattern in the angles of the polarimetric vectors. Near the core of this cluster the structure shows a semicircular pattern that we have interpreted as a reorientation of the dust particles showing the morphology of the magnetic field. We propose that a supernova event occurred some time ago and produced a shock on the local ISM. We discuss in this paper independent confirmations of this event, both from the studies on the diffuse interstellar absorptions and the results of the pre-main-sequence stars. We also show that a supernova is supported by the evolutionary status of the cluster. | en |
dc.format.extent | 349-356 | es |
dc.language | en | es |
dc.subject | Dust, extinction | es |
dc.subject | Open clusters and associations: individual (NGC 6231) | es |
dc.subject | Polarization | es |
dc.subject | Supernova remnants | es |
dc.title | Optical polarization observations of NGC 6231: Evidence for a past supernova fingerprint | en |
dc.type | Articulo | es |
sedici.identifier.other | doi:10.1086/378799 | es |
sedici.identifier.other | eid:2-s2.0-0346896429 | es |
sedici.identifier.issn | 0004-637X | es |
sedici.creator.person | Feinstein Baigorri, Carlos | es |
sedici.creator.person | Martínez, Rubén Enrique | es |
sedici.creator.person | Vergne, María Marcela | es |
sedici.creator.person | Baume, Gustavo Luis | es |
sedici.creator.person | Vázquez, Rubén Ángel | 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.description.peerReview | peer-review | es |
sedici.relation.journalTitle | The Astrophysical Journal | es |
sedici.relation.journalVolumeAndIssue | vol. 598, no. 1 | es |
sedici.rights.sherpa | * RoMEO: verde* Pre-print del autor: can* Post-print del autor: can* Versión de editor/PDF:can* Condiciones:>>On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository.>>Publisher's version/PDF may be used on any website or authors' institutional repository>>Deben reconocerse el copyright y la fuente editorial>>Debe ir enlazado a la versión de editor>>La versión de editor/PDF puede utilizarse>>Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article � a "non-exclusive licence to distribute">>Publisher last contacted on 10/02/2016>>Publisher last reviewed on 15/08/2017* Link a Sherpa: http://sherpa.ac.uk/romeo/issn/0004-637X/es/ |