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The unseen population of F- to K-type companions to hot subdwarf stars

  1. J. Girven1,*,
  2. D. Steeghs1,
  3. U. Heber2,
  4. B. T. Gänsicke1,
  5. T. R. Marsh1,
  6. E. Breedt1,
  7. C. M. Copperwheat1,
  8. S. Pyrzas1,
  9. P. Longa-Peña1

Article first published online: 13 AUG 2012

DOI: 10.1111/j.1365-2966.2012.21415.x

Issue

Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society

Volume 425, Issue 2, pages 1013–1041, 11 September 2012

Additional Information

How to Cite

Girven, J., Steeghs, D., Heber, U., Gänsicke, B. T., Marsh, T. R., Breedt, E., Copperwheat, C. M., Pyrzas, S. and Longa-Peña, P. (2012), The unseen population of F- to K-type companions to hot subdwarf stars. Monthly Notices of the Royal Astronomical Society, 425: 1013–1041. doi: 10.1111/j.1365-2966.2012.21415.x

Author Information

  1. 1

    Department of Physics, University of Warwick, Coventry

  2. 2

    Dr Remeis-Sterwarte, Astronomisches Institut der Universität Erlangen-Nürnberg, Bamberg, Germany

*E-mail: j.m.girven@warwick.ac.uk

Publication History

  1. Issue published online: 22 AUG 2012
  2. Article first published online: 13 AUG 2012
  3. Manuscript Accepted: 29 MAY 2012
  4. Manuscript Received: 29 MAY 2012

Funded by

  • NASA
  • NSF
  • Alfred P. Sloan Foundation
  • National Science Foundation
  • U.S. Department of Energy
  • National Aeronautics and Space Administration
  • Japanese Monbukagakusho, and the Max Planck Society
  • Higher Education Funding Council for England

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Table 4. Full list of objects from the C2M sample with magnitudes inside the cuts described in Table 1.

Table 8. Subdwarf and companion effective temperatures, distance estimates and magnigudes for the C2MS sample.

Table 9. Subdwarf and companion effective temperatures, distance estimates and magnigudes for the SU sample.

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