Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-16T12:53:39.678Z Has data issue: false hasContentIssue false
  • English
  • Français

Giant planets around AF and M stars

Published online by Cambridge University Press:  06 January 2014

Julien Rameau ,
Gaël Chauvin ,
Anne-Marie Lagrange ,
Philippe Delorme  and
Justine Lannier
Julien Rameau
Affiliation:
UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) UMR 5274, Grenoble, F-38041, France email: julien.rameau@obs.ujf-grenoble.fr
Gaël Chauvin
Affiliation:
UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) UMR 5274, Grenoble, F-38041, France email: julien.rameau@obs.ujf-grenoble.fr
Anne-Marie Lagrange
Affiliation:
UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) UMR 5274, Grenoble, F-38041, France email: julien.rameau@obs.ujf-grenoble.fr
Philippe Delorme
Affiliation:
UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) UMR 5274, Grenoble, F-38041, France email: julien.rameau@obs.ujf-grenoble.fr
Justine Lannier
Affiliation:
UJF-Grenoble 1 / CNRS-INSU, Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) UMR 5274, Grenoble, F-38041, France email: julien.rameau@obs.ujf-grenoble.fr
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.

We present the results of two three-year surveys of young and nearby stars to search for wide orbit giant planets. On the one hand, we focus on early-type and massive, namely β Pictoris analogs. On the other hand, we observe late type and very low mass stars, i.e., M dwarfs. We report individual detections of new planetary mass objects. According to our deep detection performances, we derive the observed frequency of giant planets between these two classes of parent stars. We find frequency between 6 to 12% but we are not able to assess a/no correlation with the host-mass.

Keywords

methods: statisticalplanetary systemsstars: individual (HD95086, J01033563-5515561)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S299: Exploring the Formation and Evolution of Planetary Systems , June 2013 , pp. 64 - 65
Copyright
Copyright © International Astronomical Union 2013 

References

Baraffe, I., Chabrier, G., Allard, F., & Hauschildt, P. 2003, Brown Dwarfs, 211, 41Google Scholar
Cameron, A. G. W. 1978, Moon and Planets, 18, 5CrossRefGoogle Scholar
Chauvin, G., Lagrange, A.-M., Beust, H., et al. 2012, A&A, 542, A41Google Scholar
Delorme, P., Lagrange, A. M., Chauvin, G., et al. 2012, A&A, 539, A72Google Scholar
Delorme, P., Gagné, J., Girard, J. H., et al. 2013, A&A, 553, L5Google Scholar
Johnson, J. A., Butler, R. P., Marcy, G. W., et al. 2007, APJ, 670, 833CrossRefGoogle Scholar
Lagrange, A.-M., Gratadour, D., Chauvin, G., et al. 2009, A&A, 493, L21Google Scholar
Marois, C., Lafrenière, D., Doyon, R., Macintosh, B., & Nadeau, D. 2006, APJ, 641, 556CrossRefGoogle Scholar
Marois, C., Macintosh, B., Barman, T., et al. 2008, Science, 322, 1348Google Scholar
Pollack, J. B., Hubickyj, O., Bodenheimer, P., et al. 1996, Icarus, 124, 62Google Scholar
Rameau, J., Chauvin, G., Lagrange, A.-M., et al. 2013, A&A, 553, A60Google Scholar
Rameau, J., Chauvin, G., Lagrange, A.-M., et al. 2013, arXiv:1305.7428Google Scholar