Abstract
Precise radial velocities from the Anglo-Australian Telescope (AAT) confirm the presence of a rare short-period planet around the K0 giant HD 121056. An independent two-planet solution using the AAT data shows that the inner planet has P = 89.1 ± 0.1 days, and m sin i = 1.35 ± 0.17 MJup. These data also confirm the planetary nature of the outer companion, with m sin i = 3.9 ± 0.6 MJup and a = 2.96 ± 0.16 AU. HD 121056 is the most-evolved star to host a confirmed multiple-planet system, and is a valuable example of a giant star hosting both a short-period and a long-period planet.
Original language | English |
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Article number | 74 |
Number of pages | 8 |
Journal | The Astrophysical Journal |
Volume | 800 |
Issue number | 1 |
DOIs | |
Publication status | Published - 10 Feb 2015 |
Externally published | Yes |
Keywords
- Planetary systems
- Stars: individual (HD 121056)
- Techniques: radial velocities