Radial velocity curves of HD 47186 and HD 181433 Virtual Observatory Resource

Authors
  1. Bouchy F.
  2. Mayor M.
  3. Lovis C.
  4. Udry S.
  5. Benz W.
  6. Bertaux J.-L.
  7. Delfosse X.,Mordasini C.
  8. Pepe F.
  9. Queloz D.
  10. Published by
    CDS
Abstract

This Letter reports on the detection of two new multiple planet systems around solar-like stars HD 47186 and HD 181433. The first system includes a hot Neptune of 22.78M_{Earth}_ at 4.08-days period and a Saturn of 0.35M_{Jup}_ at 3.7-years period. The second system includes a Super-Earth of 7.5M_{Earth}_ at 9.4-days period, a 0.64M_{Jup}_ at 2.6-years period as well as a third companion of 0.54M_{Jup}_ with a period of about 6 years. These detections increase to 20 the number of close-in low-mass exoplanets (below 0.1M_Jup_) and strengthen the fact that 80% of these planets are in a multiple planetary systems.

Keywords
  1. solar-system-planets
  2. radial-velocity
Bibliographic source Bibcode
2009A&A...496..527B
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/496/527
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/496/527
Document Object Identifer DOI
doi:10.26093/cds/vizier.34960527

Access

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https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/496/527
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/496/527
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History

2009-06-01T16:50:17Z
Resource record created
2009-06-01T16:50:17Z
Created
2017-06-20T13:17:39Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr