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New light-travel time models and orbital stability study of the proposed planetary system HU Aquarii

  1. T. C. Hinse1,2,*,
  2. J. W. Lee1,
  3. K. Goździewski3,
  4. N. Haghighipour4,
  5. C.-U. Lee1,
  6. E. M. Scullion5

Article first published online: 19 JAN 2012

DOI: 10.1111/j.1365-2966.2011.20283.x

Issue

Monthly Notices of the Royal Astronomical Society

Monthly Notices of the Royal Astronomical Society

Volume 420, Issue 4, pages 3609–3620, March 2012

Additional Information

How to Cite

Hinse, T. C., Lee, J. W., Goździewski, K., Haghighipour, N., Lee, C.-U. and Scullion, E. M. (2012), New light-travel time models and orbital stability study of the proposed planetary system HU Aquarii. Monthly Notices of the Royal Astronomical Society, 420: 3609–3620. doi: 10.1111/j.1365-2966.2011.20283.x

Author Information

  1. 1

    Korea Astronomy and Space Science Institute, 776 Daedukdae-ro, Yuseong-gu, 305-348 Daejeon, Republic of Korea

  2. 2

    Armagh Observatory, College Hill, Armagh BT61 9DG

  3. 3

    Torun Centre for Astronomy, Nicolaus Copernicus University, PL-87-100 Torun, Poland

  4. 4

    Institute for Astronomy & NASA Astrobiology Institute, University of Hawaii, HI 96822, USA

  5. 5

    Institute of Theoretical Astrophysics, University of Oslo, 0371 Oslo, Norway

* E-mail: tchinse@gmail.com

Publication History

  1. Issue published online: 1 MAR 2012
  2. Article first published online: 19 JAN 2012
  3. Accepted 2011 November 29. Received 2011 November 28; in original form 2011 October 24

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