Hostname: page-component-5c6d5d7d68-pkt8n Total loading time: 0 Render date: 2024-08-21T20:45:23.032Z Has data issue: false hasContentIssue false
  • English
  • Français

Exploring the transition into an asymmetric planetary nabulae

Published online by Cambridge University Press:  08 August 2017

Mónica W. Blanco Cárdenas ,
Roberto Vázquez ,
Hans Ulrich Kaeufl ,
Marco A. Gómez-Muñoz ,
Pedro F. Guillén ,
Martín A. Guerrero  and
Luis F. Miranda
Mónica W. Blanco Cárdenas
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Km 103 Carretera Tijuana-Ensenada 22860, Ensenada, Mexico email: [email protected]
Roberto Vázquez
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Km 103 Carretera Tijuana-Ensenada 22860, Ensenada, Mexico email: [email protected]
Hans Ulrich Kaeufl
Affiliation:
European southern Observatory, Karl Schwarchild-Str 2 85748, Garching bei Muenchen, Germany
Marco A. Gómez-Muñoz
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Km 103 Carretera Tijuana-Ensenada 22860, Ensenada, Mexico email: [email protected]
Pedro F. Guillén
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Km 103 Carretera Tijuana-Ensenada 22860, Ensenada, Mexico email: [email protected]
Martín A. Guerrero
Affiliation:
Instituto de Astofísica de Andalucía, Glorieta de la Astronomía S/N 18008, Granada, Spain
Luis F. Miranda
Affiliation:
Instituto de Astofísica de Andalucía, Glorieta de la Astronomía S/N 18008, Granada, Spain
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present studies using different observational techniques, along different frequencies, aiming to resolve and investigate jets, outflows, as well as compact and innermost regions of asymmetric planetary nebulae (PNe) and objects in transition to PN. All the information gathered allow us to explore the kinematics and other important properties of the structures that play a crucial role in the shaping of complex PNe morphologies, in particular, we explore the role of disks/tori as collimating engine of extreme axisymmetric PNe.

Keywords

Starscircumstellar materoutflows
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. 363 - 364
Copyright
Copyright © International Astronomical Union 2017 

References

Blanco Cárdenas, M., Kaeulf, H. U., Guerrero, M. A., et al. 2014, A&A, 566, A133 Google Scholar
Blanco Cárdenas, Guerrero, M. A., Ramos-Larios, G, et al. 2013, A&A, 551, A64 Google Scholar
Bujarrabal, V., Castro-Carrizo, A., Alcolea, J., et al. 2013, A&A, 557, L11 Google Scholar
Castro-Carrizo, A., Neri, R., Bujarrabal, V., et al. 2012, A&A, 545, A1 Google Scholar
Chesneau, O., Lykou, B., Balick, B., et al. 2007, A&A, 473, L29 Google Scholar
Huggins, P. J., Forveille, T., Bachiller, R., & Cox, P., 2000, ApJ, 544, 889 Google Scholar
Lykou, B., Chesneau, O., Zijlstra, A. A., et al. 2011, A&A, 527, A105 Google Scholar
Waters, L. B. F. M., Waelkens, C., van Winckel, H., et al. 1998, Nature, 67, 4679 Google Scholar