Polarimetry of R Aqr and PN M2-9

dc.contributorNavarro, S.G., Instituto de Astronomía y Meteorología, Universidad de Guadalajara, Mexico; Sabin, L., Instituto de Astronomía y Meteorología, Universidad de Guadalajara, Mexico; Ramírez, J., Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico; Hiriart, D., Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico
dc.creatorNavarro, S.G.
dc.creatorSabin, L.
dc.creatorRamirez, J.
dc.creatorHiriart, D.
dc.date.accessioned2015-11-19T18:51:50Z
dc.date.accessioned2023-07-04T04:37:44Z
dc.date.available2015-11-19T18:51:50Z
dc.date.available2023-07-04T04:37:44Z
dc.date.created2015-11-19T18:51:50Z
dc.date.issued2014
dc.identifierhttp://hdl.handle.net/20.500.12104/67047
dc.identifier10.1017/S1743921314002609
dc.identifierhttp://www.scopus.com/inward/record.url?eid=2-s2.0-84905725959&partnerID=40&md5=06fa1060d2e7b7ac57f699bf9184bde8
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7270441
dc.description.abstractThe bipolar or more complex morphology observed in planetary nebulae have been explained by two principal hypothesis: by the existence of a companion and an accreting disk or by the effects of magnetic field, (or a combination of both). Symbiotics are binary systems and some of them show morphologies similar to those observed on planetary nebulae. This fact could support the binary hypothesis for PNe. We have therefore performed polarimetric observations of symbiotic systems and some planetary nebulae in order, first to detect linear polarisation with POLIMA at the San Pedro Mártir observatory, and ultimately to prove the existence and physical properties of those disks. We present here the first results of a project dedicated to the analysis of the polarisation observed in evolved objects starting with the PN M2-9 and R Aqr. © International Astronomical Union 2014.
dc.relationProceedings of the International Astronomical Union
dc.relation9
dc.relationS302
dc.relation400
dc.relation401
dc.relationScopus
dc.titlePolarimetry of R Aqr and PN M2-9
dc.typeArticle


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