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Photoionisation effects in hydrodynamical simulations of planetary nebulae

Published online by Cambridge University Press:  08 August 2017

L. Hernández-Martínez ,
D. Estrella ,
P. F. Velázquez ,
A. Esquivel  and
A. C. Raga
L. Hernández-Martínez
Affiliation:
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, 70-543, México, D. F. México email: [email protected]
D. Estrella
Affiliation:
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, 70-543, México, D. F. México email: [email protected]
P. F. Velázquez
Affiliation:
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, 70-543, México, D. F. México email: [email protected]
A. Esquivel
Affiliation:
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, 70-543, México, D. F. México email: [email protected]
A. C. Raga
Affiliation:
Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, 70-543, México, D. F. México email: [email protected]
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Abstract

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We explored the photoionisation effects on both the proper motion and emission of planetary nebulae NGC 6302, by means of hydrodynamical simulations. We used the GUACHO code, which includes the photoionisation due to central source (Esquivel et al. 2009, Esquivel & Raga 2013). We model these PNe considering an interacting stellar fast wind with and ejected toroidally shaped slow wind (Uscanga et al. 2014). Synthetic Hα emission maps were obtained from our numerical results in order to do a comparison between the cases with and without photoionisation. Using a wavelets fittering method on our results for the ionisation case, we do not find an increase in the proper motion velocities, however we can see an accelerated expansion in both cases. For the ionisation case the Hα emission presents an increase.

Keywords

Planetary NebulaeBipolarityHydrodinamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S323: Planetary Nebulae: Multi-Wavelength Probes of Stellar and Galactic Evolution , October 2016 , pp. 350 - 351
Copyright
Copyright © International Astronomical Union 2017 

References

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