Hostname: page-component-76fb5796d-skm99 Total loading time: 0 Render date: 2024-04-27T02:21:37.016Z Has data issue: false hasContentIssue false

Misaligned spin-orbit in the XO-3 planetary system?

Published online by Cambridge University Press:  01 May 2008

G. Hébrard
Affiliation:
Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, France
F. Bouchy
Affiliation:
Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, France
F. Pont
Affiliation:
Physikalisches Institut, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
B. Loeillet
Affiliation:
Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, France Laboratoire d'Astrophysique de Marseille, Univ. de Provence, CNRS (UMR 6110), France
M. Rabus
Affiliation:
Instituto de Astrofísica de Canarias, La Laguna, Tenerife, Spain
X. Bonfils
Affiliation:
Centro de Astrofísica, Universidade do Porto, Portugal Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
C. Moutou
Affiliation:
Laboratoire d'Astrophysique de Marseille, Univ. de Provence, CNRS (UMR 6110), France
I. Boisse
Affiliation:
Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, France
X. Delfosse
Affiliation:
Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
M. Desort
Affiliation:
Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
A. Eggenberger
Affiliation:
Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
D. Ehrenreich
Affiliation:
Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
T. Forveille
Affiliation:
Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
A.-M. Lagrange
Affiliation:
Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
C. Lovis
Affiliation:
Observatoire de Genève, Université de Genève, Switzerland
M. Mayor
Affiliation:
Observatoire de Genève, Université de Genève, Switzerland
F. Pepe
Affiliation:
Observatoire de Genève, Université de Genève, Switzerland
C. Perrier
Affiliation:
Laboratoire d'Astrophysique de Grenoble, CNRS (UMR 5571), Université J. Fourier, France
N. C. Santos
Affiliation:
Centro de Astrofísica, Universidade do Porto, Portugal Observatoire de Genève, Université de Genève, Switzerland
D. Queloz
Affiliation:
Observatoire de Genève, Université de Genève, Switzerland
D. Ségransan
Affiliation:
Observatoire de Genève, Université de Genève, Switzerland
S. Udry
Affiliation:
Observatoire de Genève, Université de Genève, Switzerland
A. Vidal-Madjar
Affiliation:
Institut d'Astrophysique de Paris, UMR7095 CNRS, Université Pierre & Marie Curie, France
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The SOPHIE Consortium started a large program of exoplanets search and characterization in the Northern hemisphere with the new spectrograph SOPHIE at the 1.93-m telescope of Haute-Provence Observatory, France. The objectives of this program are to characterize the zoo of exoplanets and to bring strong constraints on their processes of formation and evolution using the radial velocity technique. We present here new SOPHIE measurements of the transiting planet host star XO-3. This allowed us to observe the Rossiter-McLaughlin effect and to refine the parameters of the planet. The unusual shape of the radial velocity anomaly during the transit provides a hint for a nearly transverse Rossiter-McLaughlin effect. The sky-projected angle between the planetary orbital axis and the stellar rotation axis should be λ = 70° ± 15° to be compatible with our observations. This suggests that some close-in planets might result from gravitational interaction between planets and/or stars rather than migration. This result requires confirmation by additional observations.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Alonso, R., Auvergne, M., Baglin, A., et al. 2008, A&A, 482, L21Google Scholar
Bakos, G. A., Shporer, A., Pal, A., et al. 2007, ApJ, 671, L173CrossRefGoogle Scholar
Barbieri, M., et al. 2008, this volumeGoogle Scholar
Barge, P., Baglin, A., Auvergne, M., et al. 2008, A&A, 482, L17Google Scholar
Bouchy, F., and the Sophie team, 2006, in 10th Anniversary of 51 Peg-b: Status of and prospects for hot Jupiter studies, eds. Arnold, L., Bouchy, F. & Moutou, C., 319Google Scholar
Bouchy, F., Queloz, D., Deleuil, M., et al. 2008, A&A, 482, L25Google Scholar
Christian, D. J., et al. , submitted to MNRAS (arXiv:0806.1482)Google Scholar
Cochran, W. D., Redfield, S., Endl, M., & Cochran, A. L., ApJ, in press (arXiv:0806.4142)Google Scholar
Collier Cameron, A., Bouchy, F., Hébrard, G., et al. 2007, MNRAS, 375, 951CrossRefGoogle Scholar
Da Silva, R., Udry, S., Bouchy, F., et al. 2008, A&A, 473, 323Google Scholar
Hébrard, G., Bouchy, F., Pont, F., et al. 2008, A&A in press (arXiv:0806.0719)Google Scholar
Johns-Krull, C. M., McCullough, P. R., Burke, C. J., et al. 2008, ApJ, 677, 657CrossRefGoogle Scholar
Joshi, Y. C., et al. , submitted to MNRAS (arXiv:0806.1478)Google Scholar
Loeillet, B., Shporer, A., Bouchy, F., et al. 2008, A&A, 481, 529Google Scholar
Narita, N., Enya, K., Sato, B., et al. 2007, PASJ, 59, 763, and this volumeCrossRefGoogle Scholar
Pollacco, D., Skillen, I., Collier Cameron, A., et al. 2008, MNRAS, 385, 1576CrossRefGoogle Scholar
Santos, N. C., Udry, S., Bouchy, F., et al. 2008, A&A in press (arXiv:0805.1019)Google Scholar
Winn, J. N., Holman, M. J., Torres, G., et al. 2008a, ApJ, in press (arXiv:0804.4475)Google Scholar