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WASP-7: a bright transiting-exoplanet ststem in the southern hemisphere
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(2009) WASP-7: a bright transiting-exoplanet ststem in the southern hemisphere. Astrophysical Journal Letters, Vol.690 (No.1). L89-L91. doi:10.1088/0004-637X/690/1/L89 Full text not available from this repository, contact author.
Official URL: http://dx.doi.org/10.1088/0004-637X/690/1/L89
Abstract
We report that a Jupiter-mass planet, WASP-7b, transits the V = 9.5 star HD 197286 every 4.95 d. This is the brightest discovery from the WASP-South transit survey so far and is currently the brightest transiting-exoplanet system in the southern hemisphere. WASP-7b is among the densest of the known Jupiter-mass planets, suggesting that it has a massive core. The planet mass is 0.96(-0.18)(+0.12) M-Jup, the radius is 0.915(-0.040)(+0.046) R-Jup, and the density is 1.26(-0.21)(+0.25) rho(Jup) (1.67(-0.28)(+0.33) g cm(-3)).
| Item Type: | Journal Article | ||||
|---|---|---|---|---|---|
| Subjects: | Q Science > QB Astronomy | ||||
| Divisions: | Faculty of Science > Physics | ||||
| Journal or Publication Title: | Astrophysical Journal Letters | ||||
| Publisher: | Institute of Physics Publishing Ltd. | ||||
| ISSN: | 2041-8213 | ||||
| Official Date: | 1 January 2009 | ||||
| Dates: |
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| Volume: | Vol.690 | ||||
| Number: | No.1 | ||||
| Number of Pages: | 3 | ||||
| Page Range: | L89-L91 | ||||
| DOI: | 10.1088/0004-637X/690/1/L89 | ||||
| Status: | Peer Reviewed | ||||
| Publication Status: | Published | ||||
| Access rights to Published version: | Restricted or Subscription Access | ||||
| Funder: | UK's Science and Technology Facilities Council |
Data sourced from Thomson Reuters' Web of Knowledge
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