Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-28T04:56:44.714Z Has data issue: false hasContentIssue false
  • English
  • Français

The Planetary Nebulae Luminosity Function (PNLF): current perspectives

Published online by Cambridge University Press:  08 August 2017

Roberto H. Méndez Open the ORCID record for Roberto H. Méndez [Opens in a new window]
Roberto H. Méndez*
Affiliation:
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA email: [email protected]
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.

This paper starts with a brief historical review about the PNLF and its use as a distance indicator. Then the PNLF distances are compared with Surface Brightness Fluctuations (SBF) distances and Tip of the Red Giant Branch (TRGB) distances. A Monte Carlo method to generate simulated PNLFs is described, leading to the last subject: recent progress in reproducing the expected maximum final mass in old stellar populations, a stellar astrophysics enigma that has been challenging us for quite some time.

Keywords

galaxies: distances and redshiftsplanetary nebulae: generalstars: AGB and post-AGBevolution
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. 298 - 302
Copyright
Copyright © International Astronomical Union 2017 

References

Bird, S., Harris, W. E., Blakeslee, J. P., & Flynn, C., 2010, A&A, 524, A71 Google Scholar
Blakeslee, J. P., Jordan, A., Mei, S., et al. 2009, ApJ, 694, 556 Google Scholar
Buzzoni, A., Arnaboldi, M., & Corradi, R. L. M., 2006, MNRAS, 368, 877 CrossRefGoogle Scholar
Ciardullo, R., 2012, Ap&SS, 341, 151 Google Scholar
Ciardullo, R., Feldmeier, J. J., Jacoby, G. H., et al. 2002, ApJ, 577, 31 Google Scholar
Ciardullo, R., Jacoby, G. H., Ford, H. C., & Neill, J. D., 1989, ApJ, 339, 53 Google Scholar
Jacoby, G. H., 1989, ApJ, 339, 39 CrossRefGoogle Scholar
Jacoby, G. H., Ciardullo, R., & Ford, H. C., 1990, ApJ, 356, 332 CrossRefGoogle Scholar
Makarov, D., Makarova, L., Rizzi, L., et al. 2006, AJ, 132, 2729 Google Scholar
Méndez, R. H. 1999, in: Heck, A. & Caputo, F. (eds.), “Post-Hipparcos Cosmic Candles”, Ap. & Space Sci. Library, 237, 161 (Kluwer)Google Scholar
Méndez, R. H., Kudritzki, R. P., Ciardullo, R., & Jacoby, G. H., 1993, A&A, 275, 534 Google Scholar
Méndez, R. H., Riffeser, A., Kudritzki, R. P., et al. 2001, ApJ, 563, 135 CrossRefGoogle Scholar
Méndez, R. H. & Soffner, T., 1997, A&A, 321, 898 Google Scholar
Méndez, R. H., Teodorescu, A. M., Schönberner, D., et al. 2008, ApJ, 681, 325 Google Scholar
Miller Bertolami, M. M., 2016, A&A, 588, A25 Google Scholar
Renzini, A. & Buzzoni, A. 1986, in: Chiosi, C. & Renzini, A. (eds.), “Spectral Evolution of Galaxies”, Ap. & Space Sci. Library, 122, 195 (Reidel)Google Scholar
Teodorescu, A. M., Méndez, R. H., Bernardi, F., et al. 2010, ApJ, 721, 369 Google Scholar
Teodorescu, A. M., Méndez, R. H., Bernardi, F., et al. 2011, ApJ, 736, 65 Google Scholar
Tonry, J., Dressler, A., Blakeslee, J. P., et al. 2001, ApJ, 546, 681 Google Scholar
Tonry, J. & Schneider, D. P., 1988, AJ, 96, 807 CrossRefGoogle Scholar