Hostname: page-component-8448b6f56d-c47g7 Total loading time: 0 Render date: 2024-04-24T07:58:19.340Z Has data issue: false hasContentIssue false
  • English
  • Français

Galactic Bulge PNe: Carbon molecules in oxygen-rich environments

Published online by Cambridge University Press:  30 August 2012

Lizette Guzmán-Ramírez ,
Albert Zijlstra ,
Roisin Níchuimín ,
Krzysztof Gesicki ,
Eric Lagadec ,
Tom J. Millar  and
Paul M. Woods
Lizette Guzmán-Ramírez
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics & Astronomy, The University of Manchester, Manchester, M13 9PL, UK email: lizette.ramirez@postgrad.manchester.ac.uk
Albert Zijlstra
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics & Astronomy, The University of Manchester, Manchester, M13 9PL, UK email: lizette.ramirez@postgrad.manchester.ac.uk
Roisin Níchuimín
Affiliation:
Jodrell Bank Centre for Astrophysics, School of Physics & Astronomy, The University of Manchester, Manchester, M13 9PL, UK email: lizette.ramirez@postgrad.manchester.ac.uk
Krzysztof Gesicki
Affiliation:
Centrum Astronomii UMK, ul.Gagarina 11, 87-100 Torun, Poland
Eric Lagadec
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str 2, 85748 Garching, Germany
Tom J. Millar
Affiliation:
Astrophysics Research Centre, Queen's University Belfast, Belfast BT7 1NN, UK
Paul M. Woods
Affiliation:
Dept. of Physics and Astronomy, University College London, Gower Street, London WC1E6BT, UK
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.

Galactic bulge planetary nebulae show evidence of mixed chemistry with emission from both silicate dust and PAHs. This mixed chemistry is unlikely to be related to carbon dredge up, as third dredge-up is not expected to occur in the low mass bulge stars. We show that the phenomenon is widespread, and is seen in 30 nebulae out of our sample of 40. A strong correlation is found between strength of the PAH bands and morphology, in particular, the presence of a dense torus. A chemical model is presented which shows that hydrocarbon chains can form within oxygen-rich gas through gas-phase chemical reactions. We conclude that the mixed chemistry phenomenon occurring in the galactic bulge planetary nebulae is best explained through hydrocarbon chemistry in an UV-irradiated, dense torus.

Keywords

planetary nebulae: generalcircumstellar matterGalaxy: bulge
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 259 - 262
Copyright
Copyright © International Astronomical Union 2012

References

Feast, M. 2007, in: Kerschbaum, F., Charbonnel, C., Wing, R. F. (eds.) Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes, 378, 479 Google Scholar
Gesicki, K. & Zijlstra, A. A. 2007, in Napiwotzki, R., Burleigh, M. R. (eds.) 15th European Workshop on White Dwarfs 372 41 Google Scholar
Guzman-Ramirez, L., Zijlstra, A. A., Níchuimín, R., et al. 2011, MNRAS, 414, 1667 CrossRefGoogle Scholar
Habing, H. J. 1996, A&AR, 7, 97 Google Scholar
Herwig, F. 2005, Annual Review of Astron and Astrophys, 43, 435 CrossRefGoogle Scholar
Houck, J. R., Roellig, T. L., van Cleve, J., et al. 2004, ApJS, 154, 18 CrossRefGoogle Scholar
Le Bertre, T., Tanaka, M., Yamamura, I., Murakami, H. 2003, A&A, 403, 943 Google Scholar
Le Petit, F., Nehmé, C., Le Bourlot, J., & Roueff, E. 2006, ApJS, 164, 506 CrossRefGoogle Scholar
Níchuimín, R. 2009, PhD thesis, Univ. ManchesterGoogle Scholar
Perea-Calderón, J. V., García-Hernández, D. A., García-Lario, P., Szczerba, R., & Bobrowsky, M. 2009, A&A, 495, L5 Google Scholar
Phillips, J. P., Cuesta, L. C., & Ramos-Larios, G. 2010, MNRAS, 409, 881 CrossRefGoogle Scholar
Savage, B. D. & Sembach, K. R. 1996, Annual Review of Astron and Astrophys, 34, 279 CrossRefGoogle Scholar
Schneider, S. E. & Buckley, D. 1996, ApJ, 459, 606 CrossRefGoogle Scholar
Uttenthaler, S., Hron, J., Lebzelter, T., et al. 2008, A&A, 478, 527 Google Scholar
Vassiliadis, E. & Wood, P. R. 1993, ApJ, 413, 641 CrossRefGoogle Scholar
Waters, L. B. F. M., Beintema, D. A., Zijlstra, A. A., et al. 1998, A&A, 331, L61 Google Scholar
Wolf, S., Henning, T., & Stecklum, B. 1999, A&A, 349, 839 Google Scholar
Woods, P. M., Nyman, L.-Å., Schöier, F. L., et al. 2005, A&A, 429, 977 Google Scholar