Our Sun lies within 300 pc of the 2.7-kpc-long sinusoidal chain of dense gas clouds known as the Radcliffe Wave. The structure's wave-like shape was discovered using 3D dust mapping, but initial kinematic searches for oscillatory motion were inconclusive. Here we present evidence that the Radcliffe Wave is oscillating through the Galactic plane while also drifting radially away from the Galactic Center. We use measurements of line-of-sight velocity for 12CO and 3D velocities of young stellar clusters to show that the most massive star-forming regions spatially associated with the Radcliffe Wave (including Orion, Cepheus, North America, and Cygnus X) move as if they are part of an oscillating wave driven by the gravitational acceleration of the Galactic potential. By treating the Radcliffe Wave as a coherently oscillating structure, we can derive its motion independently of the local Galactic mass distribution, and directly measure local properties of the Galactic potential as well as the Sun's vertical oscillation period. In addition, the measured drift of the Radcliffe Wave radially outward from the Galactic Center suggests that the cluster whose supernovae ultimately created today's expanding Local Bubble may have been born in the Radcliffe Wave.
A study of the spatial evolution of the Radcliffe wave in a sample of young open star clusters
Central Astronomical Observatory of the Russian Academy of Sciences(俄罗斯科学院中央天文台);Pulkovo Institute of Applied Astronomy of the Russian Academy of Sciences(俄罗斯科学院普尔科沃应用天文学研究所)
The Radcliffe Wave as traced by young open clusters: Stellar parameters, activity indicators, and abundances of solar-type members of eight young clusters
Parameters of the Galactic Spiral Density Wave from Masers with Parallax Errors Less Than 10%
本文用VLBI测量的三角视差和自行研究了银河系脉泽和射电星的运动学。我们考虑了相对三角视差误差小于10%的脉泽,并由此确定了银河系的自转参数。特别是,银河系在太阳距离$R_0$处的线旋转速度已被发现为$244.4\pm4.3$ km s $^{-1}$(对于采用的$R_0=8.1\pm0.1$ kpc)。我们已经进行了联合和单独的径向,剩余的切向和垂直脉泽速度的频谱分析。例如,我们从垂直脉泽速度估算了速度扰动幅度$f_W=5.2\pm1.5$ km s $^{-1}$,波长为$λ_W=2.6\pm0.7$ kpc,讨论了螺旋密度波对垂直恒星速度的影响。基于104个距太阳3 kpc以内的脉泽,作为联合解的结果,我们估算了银河系螺旋密度波$f_R=6.7\pm1.1$的径向、切向速度扰动、扰动波长和太阳相位.我们已经证实了拉德克利夫波的存在,属于本地臂的脉泽和射电星的空间分布。