Hostname: page-component-848d4c4894-sjtt6 Total loading time: 0 Render date: 2024-06-24T01:15:19.343Z Has data issue: false hasContentIssue false
  • English
  • Français

Spectral analysis of PG 1034+001, the exciting star of Hewett 1

Published online by Cambridge University Press:  30 August 2012

Marin Mahsereci ,
Ellen Ringat ,
Thomas Rauch ,
Klaus Werner  and
Jeffrey W. Kruk
Marin Mahsereci
Affiliation:
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany email: maren.mahsereci@astro.uni-tuebingen.de
Ellen Ringat
Affiliation:
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany email: maren.mahsereci@astro.uni-tuebingen.de
Thomas Rauch
Affiliation:
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany email: maren.mahsereci@astro.uni-tuebingen.de
Klaus Werner
Affiliation:
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany email: maren.mahsereci@astro.uni-tuebingen.de
Jeffrey W. Kruk
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.
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.

PG 1034+001 is an extremely hot, helium-rich DO-type star that excites the planetary nebula Hewett 1 and large parts of the surrounding interstellar medium. We present preliminary results of an ongoing spectral analysis by means of non-LTE model atmospheres that consider most elements from hydrogen to nickel. This analysis is based on high-resolution ultraviolet (FUSE, IUE) and optical (VLT/UVES, Keck) data. The results are compared with those of PG 1034+001's spectroscopic twin, the DO star PG 0038+199.

Keywords

stars: abundancesstars: AGB and post-AGBstars: atmospheresstars: evolutionstars: individual (PG 1034+001, PG 0038+199)planetary nebulae: individual (Hewett 1)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S283: Planetary Nebulae: An Eye to the Future , July 2011 , pp. 426 - 427
Copyright
Copyright © International Astronomical Union 2012

References

Dreizler, S. & Werner, K. 1996, A&A, 314, 217 Google Scholar
Hewett, P. C., Irwin, M. J., Skillman, E. D., et al. 2003, ApJ, 599, L37 CrossRefGoogle Scholar
Rauch, T., Kerber, F., & Pauli, E.-M. 2004, A&A, 417, 647 Google Scholar
Werner, K. & Herwig, F. 2006, PASP, 118, 183 CrossRefGoogle Scholar
Werner, K., Dreizler, S., & Wolff, B. 1995, A&A, 298, 567 Google Scholar
Wesemael, F., Green, R. F., & Liebert, J. 1985, ApJ, 307, 659 Google Scholar