Abstract
Multiplanet systems exhibit a diversity of architectures that diverge from the solar system and contribute to the topic of exoplanet demographics. Radial velocity (RV) surveys form a crucial component of exoplanet surveys, as their long observational baselines allow for searches for more distant planetary orbits. This work provides a significantly revised architecture for the multiplanet system HD 134606 using both HARPS and UCLES RVs.
Original language | English |
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Article number | 155 |
Journal | Astronomical Journal |
Volume | 167 |
Issue number | 4 |
Number of pages | 17 |
ISSN | 0004-6256 |
DOIs | |
Publication status | Published - 2024 |
Keywords
- Exoplanets
- Exoplanet detection methods
- Exoplanet dynamics
- Exoplanet systems
- Radial velocity
- Photometry
- High contrast techniques
- Astrometry
- Orbits
- Stellar activity