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25 April 2024
 
  » arxiv » astro-ph/0305434

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The CORALIE survey for southern extra-solar planets XI. The return of the giant planet orbiting HD192263
N.C. Santos ; S. Udry ; M. Mayor ; D. Naef ; F. Pepe ; D. Queloz ; G. Burki ; N. Cramer ; B. Nicolet ;
Date 22 May 2003
Journal Astron.Astrophys. 406 (2003) 373-382
Subject astro-ph
Affiliation1 and 2), S. Udry , M. Mayor , D. Naef , F. Pepe , D. Queloz , G. Burki , N. Cramer , B. Nicolet ( Geneva Observatory, Switzerland, Observatory of Lisbon, Portugal
AbstractThe presence of a planet around the K dwarf HD192263 was recently called into question by the detection of a periodic photometric signal with the same period as the one observed in radial velocity. In this paper, we investigate this possibility, using a combination of radial-velocity, photometry, and bisector measurements obtained simultaneously. The results show that while the observed radial-velocity variation is always very stable in phase, period, and amplitude, the photometric signal changes with time. The combined information strongly suggests that the observed radial-velocity variation is being produced by the presence of a planet, as firstly proposed. The photometric variations are either not connected to the planetary companion, or can eventually be induced by the interaction between the planet and the star. Finally, the radial-velocity data further show the presence of a long term trend, whose origin, still not clear, might be related to the presence of another companion to the system.
Source arXiv, astro-ph/0305434
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