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The Third Body in the Eclipsing Binary AV CMi: Hot Jupiter or Brown Dwarf?

  • Alexios Liakos (a1), Dimitris Mislis (a2) and Panagiotis Niarchos (a1)
Abstract

New transit light curves of the third body in the system AV CMi have been obtained. The eclipsing pair's light curves were re-analysed with the W-D code and new absolute elements were derived for the two components. Moreover the new light curves (together with those given by Liakos & Niarchos 2010) of the third body transiting one of the components were analysed with the Photometric Software for Transits (PhoS-T). The results from both analyses are combined with the aim to study the nature of the third component.

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Copyright
References
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Claret, A. 2004, A&A, 428, 1001
Liakos, A. & Niarchos, P. 2010, ASP-CS, 424, 208
Mislis, D., et al. , 2011, AIP-CP, in press
Prša, A. & Zwitter, T. 2005, ApJ, 628, 426
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Proceedings of the International Astronomical Union
  • ISSN: 1743-9213
  • EISSN: 1743-9221
  • URL: /core/journals/proceedings-of-the-international-astronomical-union
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