Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-28T01:42:06.116Z Has data issue: false hasContentIssue false
  • English
  • Français

The ionization of galaxies by their planetary nebulae

Published online by Cambridge University Press:  30 August 2012

Grażyna Stasińska
Grażyna Stasińska*
Affiliation:
LUTH, Observatoire de Paris, CNRS, Université Paris Diderot; Place Jules Janssen 92190 Meudon, France email: grazyna.stasinsa@obspm.fr
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.

Recent studies have shown that nuclei of planetary nebulae and their remnants (dubbed HOLMES for “hot low-mass evolved stars”) can easily explain two long-standing problems of extragalactic astronomy: the observed emission-line spectra of ellipticals and LINER-like galaxies and the ionization and heating of the diffuse interstellar medium in spirals. They are summarized in this contribution. It is emphasized that the computation of grids of stellar evolution models until the white dwarf stage is essential not only for the study of planetary nebulae but also for the study of the ionization of galaxies.

Keywords

Planetary nebulae: generalstars: AGB and post-AGBgalaxies: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 239 - 242
Copyright
Copyright © International Astronomical Union 2012

References

Annibali, F., et al. , 2010, A&A, 519, A40 Google Scholar
Baldwin, J. A., Phillips, M. M., & Terlevich, R., 1981, PASP, 93, 5 CrossRefGoogle Scholar
Binette, L., Magris, C. G., Stasińska, G., & Bruzual, A. G., 1994, A&A, 292, 13 Google Scholar
Ciardullo, R., Sigurdsson, S., Feldmeier, J. J., & Jacoby, G. H., 2005, AIPC, 804, 292 Google Scholar
Cid Fernandes, R., Mateus, A., Sodré, L., Stasińska, G., & Gomes, J. M., 2005, MNRAS, 358, 363 CrossRefGoogle Scholar
Cid Fernandes, R., Stasińska, G., Schlickmann, M. S., Mateus, A., Vale Asari, N., Schoenell, W., & Sodré, L., 2010, MNRAS, 403, 1036 CrossRefGoogle Scholar
Cid Fernandes, R., Stasińska, G., Mateus, A. & Vale Asari, N., 2011, MNRAS, 413, 1687 CrossRefGoogle Scholar
Flores-Fajardo, N., Morisset, C., Stasińska, G., & Binette, L., 2011, MNRAS, 415, 2182 CrossRefGoogle Scholar
Haffner, L. M., et al. , 2009, RvMP, 81, 969 Google Scholar
Heckman, T. M., 1980, A&A, 87, 152 Google Scholar
Ho, L. C., 2008, ARA&A, 46, 475 Google Scholar
Jacoby, G. H., Ciardullo, R., & Feldmeier, J. J., 1999, ASPC, 167, 175 Google Scholar
Kauffmann, G., et al. , 2003, MNRAS, 346, 1055 CrossRefGoogle Scholar
Kewley, L. J., Groves, B., Kauffmann, G., & Heckman, T., 2006, MNRAS, 372, 961 CrossRefGoogle Scholar
Marigo, P., Girardi, L., Weiss, A., Groenewegen, M. A. T., & Chiosi, C., 2004, A&A, 423, 995 Google Scholar
Sarzi, M., et al. , 2010, MNRAS, 402, 2187 CrossRefGoogle Scholar
Stasińska, G., 2007, arXiv, arXiv:0704.0348Google Scholar
Stasińska, G., et al. , 2008, MNRAS, 391, L29 CrossRefGoogle Scholar
Weiss, A., & Ferguson, J. W., 2009, A&A, 508, 1343 Google Scholar
York, D. G., et al. , 2000, AJ, 120, 1579 CrossRefGoogle Scholar