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Near IR and visual polarimetry of the Planetary Nebula M2-9

Published online by Cambridge University Press:  30 December 2019

Silvana G. Navarro ,
Omar Serrano ,
Abraham Luna ,
Rangaswami Devaraj ,
Luis J. Corral Open the ORCID record for Luis J. Corral [Opens in a new window] ,
Julio Ramírez Vélez  and
David Hiriart
Silvana G. Navarro
Affiliation:
Instituto de Astronomía y Meteorología, Universidad de Guadalajara, 44130 Guadalajara, Jal., México emails: [email protected], [email protected]
Omar Serrano
Affiliation:
Instituto Nacional de Astrofísica Óptica y Electrónica, 72840 Puebla, Pue., México emails: [email protected], [email protected]
Abraham Luna
Affiliation:
Instituto Nacional de Astrofísica Óptica y Electrónica, 72840 Puebla, Pue., México emails: [email protected], [email protected]
Rangaswami Devaraj
Affiliation:
Instituto Nacional de Astrofísica Óptica y Electrónica, 72840 Puebla, Pue., México emails: [email protected], [email protected]
Luis J. Corral
Affiliation:
Instituto de Astronomía y Meteorología, Universidad de Guadalajara, 44130 Guadalajara, Jal., México emails: [email protected], [email protected]
Julio Ramírez Vélez
Affiliation:
Instituto de Astronomía, sede Ensenada, Universidad Nacional Autónoma de México, Ensenada Baja California, México emails: [email protected], [email protected]
David Hiriart
Affiliation:
Instituto de Astronomía, sede Ensenada, Universidad Nacional Autónoma de México, Ensenada Baja California, México emails: [email protected], [email protected]
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Abstract

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Bipolar and more complex morphologies observed in planetary nebulae have been explained by two principal hypotheses: by the existence of a companion producing a circumstellar disk, by the effects of a magnetic field, or by a combination of both. The polarimetric analysis of these objects could give information about the presence of dust grains aligned with any preferential direction, due to a magnetic field or to the action of radiative torques (RAT). We performed polarimetric observations of some planetary nebulae in order to detect linear polarization and (in the best scenario) to detect the signature of an accretion disk in these objects. We observed in the visual region with POLIMA at the San Pedro Mártir observatory, and with POLICAN the NIR polarimeter in the Guillermo Haro observatory. We present the result of these observations in one of these objects: the PN M2-9.

Keywords

Polarizationstars: magnetic fieldsISM: Planetary Nebulae: individual: M2-9
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S343: Why Galaxies Care About AGB Stars: A Continuing Challenge through Cosmic Time , August 2018 , pp. 480 - 482
Copyright
© International Astronomical Union 2019 

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