Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-30T21:27:43.940Z Has data issue: false hasContentIssue false
  • English
  • Français

GLMP 160 – the first [WR] star in a binary

Published online by Cambridge University Press:  30 August 2012

Marcin Hajduk ,
Peter A. M. van Hoof  and
Albert A. Zijlstra
Marcin Hajduk
Affiliation:
Nicolaus Copernicus Astronomical Center, ul. Rabiańska 8, 87-100 Toruń, Poland
Peter A. M. van Hoof
Affiliation:
Royal Observatory of Belgium, Ringlaan 3, 1180 Brussels, Belgium
Albert A. Zijlstra
Affiliation:
Jodrell Bank Centre for Astrophysics, Alan Turing Building, Manchester M13 9PL, UK
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.

We discuss the results of the search for [WR] central stars in binary systems. GLMP 160 is the first [WR] central star in a binary system known. We analyze photometry, spectroscopy and imaging of this system.

Keywords

binaries: closestars: evolutionplanetary nebulae: 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. 382 - 383
Copyright
Copyright © International Astronomical Union 2012

References

Hajduk, M., Zijlstra, A. A., & Gesicki, K. 2010, MNRAS, 406, 626 CrossRefGoogle Scholar
Miszalski, B., Acker, A., Moffat, A. F. J., Parker, Q. A., & Udalski, A. 2009, A&A, 496, 813 Google Scholar
Pereira, C. B. & Machado, M. 2003, A&A, 407, 311 Google Scholar
Pojmański, G. 2002, AcA, 52, 397 Google Scholar