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The evolution of naked helium stars with a neutron star companion in close binary systems

  1. J. D. M. Dewi1,2,3,*,
  2. O. R. Pols4,†,*,
  3. G. J. Savonije1,
  4. E. P. J. Van Den Heuvel1

Article first published online: 20 NOV 2002

DOI: 10.1046/j.1365-8711.2002.05257.x

Issue

Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society

Volume 331, Issue 4, pages 1027–1040, April 2002

Additional Information

How to Cite

Dewi, J. D. M., Pols, O. R., Savonije, G. J. and Van Den Heuvel, E. P. J. (2002), The evolution of naked helium stars with a neutron star companion in close binary systems. Monthly Notices of the Royal Astronomical Society, 331: 1027–1040. doi: 10.1046/j.1365-8711.2002.05257.x

Author Information

  1. 1

    1Astronomical Institute Anton Pannekoek, University of Amsterdam, Kruislaan 403, NL-1098 SJ Amsterdam, the Netherlands

  2. 2

    2Bosscha Observatory, Lembang 40391, Bandung, Indonesia

  3. 3

    3Department of Astronomy, Institut Teknologi Bandung, Jl. Ganesha 10, Bandung 40132, Indonesia

  4. 4

    4Department of Mathematics, PO Box 28M, Monash University, Clayton, Victoria 3800, Australia

  1. †

    †Present address: Astronomical Institute, University of Utrecht, Postbus 80000, 3508 TA Utrecht, the Netherlands.

*jasinta@astro.uva.nlJDMD
O.R.Pols@astro.uu.nlORP

  1. †

    †Present address: Astronomical Institute, University of Utrecht, Postbus 80000, 3508 TA Utrecht, the Netherlands.

  2. 1 An evolutionary channel for the formation of a double neutron star binary similar to the standard scenario was also proposed by ‡. They predicted a helium star mass of 2 M⊙ as the limiting mass for white dwarf/neutron star formation.

  3. 2 We could not follow the subsequent evolution in MHe≤2.5 M⊙ stars. However, we expect that these stars will undergo the same phenomenon as is found in the more massive ones.

Publication History

  1. Issue published online: 20 NOV 2002
  2. Article first published online: 20 NOV 2002
  3. Accepted 2001 December 10. Received 2001 December 7; in original form 2001 October 1

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