DMPP-4: candidate sub-Neptune mass planets orbiting a naked-eye star
DMPP-4: candidate sub-Neptune mass planets orbiting a naked-eye star
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DMPP-4:围绕肉眼恒星运行的候选亚海王星质量行星
DOI:
10.1093/mnras/stad2109
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发表时间:
2023
影响因子:
4.8
通讯作者:
Barnes J
中科院分区:
文献类型:
--
作者:
Barnes J
We present radial velocity measurements of the very bright (V∼ 5.7) nearby F star, DMPP-4 (HD 184960). The anomalously low CaiiH&K emission suggests mass-loss from planets orbiting a low activity host star. Periodic radial velocity variability with ∼10 m s−1amplitude is found to persist over a >4 yr time-scale. Although the non-simultaneous photometric variability in fourTESSsectors supports the view of an inactive star, we identify periodic photometric signals and also find spectroscopic evidence for stellar activity. We used a posterior sampling algorithm that includes the number of Keplerian signals,Np, as a free parameter to test and compare (1) purely Keplerian models (2) a Keplerian model with linear activity correlation and (3) Keplerian models with Gaussian processes. A preferred model, with one Keplerian and quasi-periodic Gaussian process indicates a planet with a period ofd and corresponding minimum mass ofM⊕. Without further high-time resolution observations over a longer time-scale, we cannot definitively rule out the purely Keplerian model with two candidates planets withd, minimum massM⊕andd and corresponding minimum mass ofM⊕. The candidate planets lie in the region below the lower-envelope of the Neptune Desert. Continued mass-loss may originate from the highly irradiated planets or from an as yet undetected body in the system.