Hostname: page-component-8448b6f56d-c4f8m Total loading time: 0 Render date: 2024-04-24T03:50:26.157Z Has data issue: false hasContentIssue false
  • English
  • Français

Dust in planetary nebulae

Published online by Cambridge University Press:  08 August 2017

G. C. Sloan Open the ORCID record for G. C. Sloan [Opens in a new window]
G. C. Sloan*
Affiliation:
Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218, USA Department of Physics and Astronomy, University of North Carolina, Chapel Hill, NC 27599-3255, USA Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14850-6801, USA
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.

Infrared spectra from the Spitzer Space Telescope trace the evolution of carbon-rich dust from the asymptotic giant branch (AGB) to young planetary nebulae (PNe). On the AGB, amorphous carbon dominates the dust, but SiC and MgS also appear. In more evolved systems with warmer central stars, the spectra reveal the unidentified 21 μm feature, features from aliphatic hydrocarbons, and spectra from polycyclic aromatic hydrocarbons (PAHs), often with shifted feature positions indicative of the presence of aliphatics. More evolved systems with hot central stars show more typical PAH spectra, along with fullerenes and/or an emission feature known as the big-11 feature at ~11 μm. This features arises from a combination of SiC and PAHs, and it is usually accompanied by a shoulder at 18 μm, which while unidentified might be from cool silicate grains. The strong emission from MgS and SiC in young PNe probably arises from coatings on carbonaceous grains.

Keywords

stars: AGB and post-AGBplanetary nebulae: generaldust
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. 121 - 127
Copyright
Copyright © International Astronomical Union 2017 

References

Allamandola, L. J., Tielens, A. G. G. M., & Barker, J. R., 1985, ApJ, 290, L25 Google Scholar
Allamandola, L. J., Tielens, A. G. G. M., & Barker, J. R., 1989, ApJS, 71, 733 Google Scholar
Bernard-Salas, J., Peeters, E., Sloan, G., et al. 2009, ApJ, 699, 1541 CrossRefGoogle Scholar
Cami, J. 2017, these proceedingsGoogle Scholar
Cerrigone, L., Hora, J. L., Umana, G., et al. 2011, ApJ, 738, 121 Google Scholar
Chiar, J. E., Pendleton, Y. J., Geballe, T. R., & Tielens, A. G. G. M., 1998, ApJ, 507, 281 Google Scholar
Forrest, W. J., Houck, J. R., & McCarthy, J. F., 1981, ApJ, 248, 195 Google Scholar
Geballe, T. R., Tielens, A. G. G. M., Kwok, S., & Hrivnak, B. J., 1992, ApJ, 387, L89 Google Scholar
Geballe, T. R. & van der Veen, W. E. C. J., 1990, A&A, 235, L9 Google Scholar
Gillett, F. C., Forrest, W. J., & Merrill, K. M., 1973, ApJ, 183, 87 Google Scholar
Goebel, J. H. & Moseley, S. H., 1985, ApJ, 290, L35 Google Scholar
Gutenkunst, S., Bernard-Salas, J., Pottasch, S. R., Sloan, G. C., Houck, J. R., 2008, ApJ, 680, 1206 Google Scholar
Guzman-Ramirez, L., Lagadec, E., Jones, D., Zijlstra, A. A., & Gesicki, K., 2014, MNRAS, 441, 364 Google Scholar
Guzman-Ramirez, L., Lagadec, E., Wesson, R., et al. 2015, MNRAS, 451, L1 Google Scholar
Houck, J. R., Roellig, T. L., van Cleve, J., et al. 2004, ApJS, 154, 18 CrossRefGoogle Scholar
Kwok, S., Hrivnak, B. J., & Volk, K. M., 1989, ApJ, 345, L51 Google Scholar
Lagadec, E., Zijlstra, A. A., Sloan, G. C., et al. 2007, MNRAS, 376, 1270 CrossRefGoogle Scholar
Leger, A. & Puget, J. L., 1984, A&A, 137, L5 Google Scholar
Leisenring, J. M., Kemper, F., & Sloan, G. C., 2008, ApJ, 681, 1557 Google Scholar
Lombaert, R., de Vries, B. L., de Koter, A., et al. 2012, A&A, 544, L18 Google Scholar
Matsuura, M., Bernard-Salas, J., Lloyd Evans, T., et al. 2014, MNRAS, 439, 1472 Google Scholar
Peeters, E., Hony, S., Van Kerckhoven, C., et al. 2002, A&A, 390, 1089 Google Scholar
Pino, T., Dartois, E., Cao, A.-T., et al. 2008, A&A, 490, 665 Google Scholar
Sloan, G. C., Jura, M., & Duley, W. W., et al. 2007, ApJ, 664, 1144 Google Scholar
Sloan, G. C., Kraemer, K. E., Matsuura, M., et al. 2006, ApJ, 645, 1118 Google Scholar
Sloan, G. C., Kraemer, K. E., McDonald, I., et al. 2016, ApJ, 826, 44 CrossRefGoogle Scholar
Sloan, G. C., Lagadec, E., Zijlstra, A. A., et al. 2014, ApJ, 791, 28 Google Scholar
Volk, K., Hrivnak, B. J., Matsuura, M., et al. ApJ, 735, 127 Google Scholar
Werner, M. W., Roellig, T. L., Low, F. J., et al. 2004, ApJS, 154, 1 Google Scholar
Zhang, K., Jiang, B. W., & Li, A., 2009, ApJ, 702, 680 Google Scholar
Zhukovska, S. & Gail, H.-P., 2008, A&A, 486, 229 Google Scholar
Zijlstra, A. A., Matsuura, M., Wood, P. R., et al. 2006, MNRAS, 370, 1961 Google Scholar