Hostname: page-component-745bb68f8f-kw2vx Total loading time: 0 Render date: 2025-01-08T14:03:07.073Z Has data issue: false hasContentIssue false
  • English
  • Français

Semi-dynamic Modeling of Shell Formation for V4334 Sgr (Sakurai): An Online Probe for Early PNe Evolution?

Published online by Cambridge University Press:  26 May 2016

Stefan Kimeswenger
Stefan Kimeswenger*
Affiliation:
Institut für Astrophysik, Leopold–Franzens Universität Innsbruck, Technikerstraße 25, A-6020 Innsbruck, AUSTRIA

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.

The central star V4334 Sgr (Sakurai's Nova) of the planetary nebula PN G010.4+04.4 underwent in 1995–1996 the rare event of a very late helium flash shell burning. The rapid formation of a dust shell allows a precise model, basing on the dust formation history instead of the commonly used average dust formation rate and mass loss. The model applies a complete dust grain size distribution, and transiently heated grains. Only the fitting of the visual light curve gives already the complete spectral energy distribution (SED) model. No adjustment with the infrared data points is needed.

Type
Part VII: Nebular Morphology and Dynamics
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 529 - 530
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Borkowski, K.J., Harrington, J.P., Blair, W.P., & Bregman, J.D. 1994, ApJ, 235, 722 CrossRefGoogle Scholar
Clayton, G.C., & deMarco, O. 1997, AJ, 114, 2679 CrossRefGoogle Scholar
Iben, I., Kaler, J.B., Truran, J.W., & Renzini, R. 1983, ApJ, 264, 605 CrossRefGoogle Scholar
Kerber, F., Gratl, H., Kimeswenger, S., & Roth, M. 1998, Ap&SS, 255, 279 Google Scholar
Kerber, F., Blommaert, J.A.D.L., Groenewegen, M.A.T., Kimeswenger, S., Käufl, H.-U., & Asplund, M., 1999, A&A, 350, L27 Google Scholar
Kimeswenger, S. 2001, Ap&SS, in press, astro-ph/0105119 Google Scholar
Kimeswenger, S., Gratl, H., Kerber, F., et al. 1997, IAUC 6608 Google Scholar
Kimeswenger, S., Kerber, F., & Weinberger, R. 1998, MNRAS, 296, 614 Google Scholar
Kipper, T. 1999, Baltic Astronomy, 8, 483 Google Scholar
Koller, J., & Kimeswenger, S. 2000, in ASP Conf. Ser. Vol. 196, Thermal Emission Spectroscopy and Analysis of Dust, Disks, and Regoliths, ed. Sitko, M.L., Sprague, A.L. & Lynch, D.K. (San Francisco: ASP), 23 Google Scholar
Koller, J., & Kimeswenger, S. 2001, ApJ, 559, 419 CrossRefGoogle Scholar