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The very fast evolution of Sakurai's object

Published online by Cambridge University Press:  08 August 2017

G. C. Van de Steene ,
P. A. M. van Hoof ,
S. Kimeswenger ,
A. A. Zijlstra ,
A. Avison ,
L. Guzman-Ramirez ,
M. Hajduk  and
F. Herwig
G. C. Van de Steene
Affiliation:
Royal Observatory of Belgium, Astronomy & Astrophysics, Ringlaan 3, Brussels, Belgium email: [email protected]
P. A. M. van Hoof
Affiliation:
Royal Observatory of Belgium, Astronomy & Astrophysics, Ringlaan 3, Brussels, Belgium email: [email protected]
S. Kimeswenger
Affiliation:
Universidad Católica del Norte, Antofagasta, Chile
A. A. Zijlstra
Affiliation:
Jodrell Bank Centre for Astrophysics, Manchester, UK
A. Avison
Affiliation:
Jodrell Bank Centre for Astrophysics, Manchester, UK
L. Guzman-Ramirez
Affiliation:
Sterrewacht, Universiteit Leiden, The Netherlands
M. Hajduk
Affiliation:
Nicolaus Copernicus Astronomical Center, Torun, Poland
F. Herwig
Affiliation:
University of Victoria, Victoria, Canada
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Abstract

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V4334 Sgr (a.k.a. Sakurai's object) is the central star of an old planetary nebula that underwent a very late thermal pulse a few years before its discovery in 1996. We have been monitoring the evolution of the optical emission line spectrum since 2001. The goal is to improve the evolutionary models by constraining them with the temporal evolution of the central star temperature. In addition the high resolution spectral observations obtained by X-shooter and ALMA show the temporal evolution of the different morphological components.

Keywords

planetary nebulae: individual (V4334 Sgr)evolutionStars: AGB and post-AGBcircumstellar matter
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. 380 - 381
Copyright
Copyright © International Astronomical Union 2017 

References

Chesneau, O., Clayton, G. C., Lykou, F., et al., 2009, A&A, 493, L17 Google Scholar
Eyres, S. P. S., Smalley, B., Geballe, T. R., et al., 1999, MNRAS, 307, L11 CrossRefGoogle Scholar
Hajduk, M., Zijlstra, A. A., Herwig, F., et al., 2005, Science, 308, 231 CrossRefGoogle Scholar
Herwig, F., Pignatari, M., Woodward, P. R., et al., 2011, ApJ, 727, 89 CrossRefGoogle Scholar
Herwig, F., Woodward, P. R., Lin, P.-H., Knox, M., & Fryer, C., 2014, ApJ, 792, L3 CrossRefGoogle Scholar
Hinkle, K. H. & Joyce, R. R., 2014, ApJ, 785, 146 Google Scholar
Kerber, F., Pirzkal, N., De Marco, O., et al., 2002, ApJ, 581, L39 Google Scholar
Lawlor, T. M. & MacDonald, J., 2003, ApJ, 583, 913 Google Scholar
Miller Bertolami, M. M., Althaus, L. G., Serenelli, A. M., & Panei, J. A., 2006, A&A, 449, 313 Google Scholar
Nakano, S., Sakurai, Y., Hazen, M., et al., 1996, IAU Circ., 6322, 1 Google Scholar
van Hoof, P. A. M., Hajduk, M., Zijlstra, A. A., et al., 2007, A&A, 471, L9 Google Scholar
van Hoof, P. A. M., Hajduk, M., Zijlstra, A. A., et al., 2008, ASP Conf. Ser., vol. 391, 155 Google Scholar